Planck intermediate results XVIII the millimetre and sub-millimetre emission from planetary nebulae

M. Arnaud; F. Atrio-Barandela; J. Aumont; C. Baccigalupi; A. J. Banday; R. B. Barreiro; E. Battaner; K. Benabed; A. Benoit-Lévy; J. P. Bernard; M. Bersanelli; P. Bielewicz; A. Bonaldi; J. R. Bond; J. Borrill; F. R. Bouchet; C. S. Buemi; C. Burigana; J. F. Cardoso; S. Casassus; A. Catalano; L. Cerrigone; A. Chamballu; H. C. Chiang; S. Colombi; L. P.L. Colombo; F. Couchot; B. P. Crill; A. Curto; F. Cuttaia; R. D. Davies; R. J. Davis; P. De Bernardis; A. De Rosa; G. De Zotti; J. Delabrouille; C. Dickinson; J. M. Diego; S. Donzelli; O. Doré; X. Dupac; T. A. Enßlin; H. K. Eriksen; F. Finelli; M. Frailis; E. Franceschi; S. Galeotta; K. Ganga; M. Giard; J. González-Nuevo; K. M. Górski; A. Gregorio; A. Gruppuso; F. K. Hansen; D. L. Harrison; S. R. Hildebrandt; E. Hivon; W. A. Holmes; J. L. Hora; A. Hornstrup; W. Hovest; K. M. Huffenberger; T. R. Jaffe; W. C. Jones; M. Juvela; E. Keihänen; R. Keskitalo; T. S. Kisner; J. Knoche; M. Kunz; H. Kurki-Suonio; A. Lähteenmäki; J. M. Lamarre; A. Lasenby; C. R. Lawrence; R. Leonardi; P. Leto; P. B. Lilje; M. Linden-Vørnle; M. López-Caniego; J. F. Macías-Pérez; B. Maffei; D. Maino; N. Mandolesi; P. G. Martin; S. Masi; M. Massardi; S. Matarrese; P. Mazzotta; L. Mendes; A. Mennella; M. Migliaccio; M. A. Miville-Deschênes; A. Moneti; L. Montier; G. Morgante; D. Mortlock; D. Munshi; J. A. Murphy; P. Naselsky; F. Nati; P. Natoli; F. Noviello; D. Novikov; I. Novikov; L. Pagano; F. Pajot; R. Paladini; D. Paoletti; M. Peel; O. Perdereau; F. Perrotta; F. Piacentini; M. Piat; D. Pietrobon; S. Plaszczynski; E. Pointecouteau; G. Polenta; L. Popa; G. W. Pratt; P. Procopio; S. Prunet; J. L. Puget; J. P. Rachen; M. Reinecke; M. Remazeilles; S. Ricciardi; T. Riller; I. Ristorcelli; G. Rocha; C. Rosset; G. Roudier; J. A. Rubiño-Martín; B. Rusholme; M. Sandri; G. Savini; D. Scott; L. D. Spencer; V. Stolyarov; D. Sutton; A. S. Suur-Uski; J. F. Sygnet; J. A. Tauber; L. Terenzi; L. Toffolatti; M. Tomasi; C. Trigilio; M. Tristram; T. Trombetti; M. Tucci; G. Umana; J. Valiviita; B. Van Tent; P. Vielva; F. Villa; L. A. Wade; B. D. Wandelt; A. Zacchei; A. Zijlstra; A. Zonca

doi:10.1051/0004-6361/201423836

Planck intermediate results XVIII the millimetre and sub-millimetre emission from planetary nebulae

M. Arnaud, F. Atrio-Barandela, J. Aumont, C. Baccigalupi, A. J. Banday, R. B. Barreiro, E. Battaner, K. Benabed, A. Benoit-Lévy, J. P. Bernard, M. Bersanelli, P. Bielewicz, A. Bonaldi, J. R. Bond, J. Borrill, F. R. Bouchet, C. S. Buemi, C. Burigana, J. F. Cardoso, S. CasassusA. Catalano, L. Cerrigone, A. Chamballu, H. C. Chiang, S. Colombi, L. P.L. Colombo, F. Couchot, B. P. Crill, A. Curto, F. Cuttaia, R. D. Davies, R. J. Davis, P. De Bernardis, A. De Rosa, G. De Zotti, J. Delabrouille, C. Dickinson, J. M. Diego, S. Donzelli, O. Doré, X. Dupac, T. A. Enßlin, H. K. Eriksen, F. Finelli, M. Frailis, E. Franceschi, S. Galeotta, K. Ganga, M. Giard, J. González-Nuevo, K. M. Górski, A. Gregorio, A. Gruppuso, F. K. Hansen, D. L. Harrison, S. R. Hildebrandt, E. Hivon, W. A. Holmes, J. L. Hora, A. Hornstrup, W. Hovest, K. M. Huffenberger, T. R. Jaffe, W. C. Jones, M. Juvela, E. Keihänen, R. Keskitalo, T. S. Kisner, J. Knoche, M. Kunz, H. Kurki-Suonio, A. Lähteenmäki, J. M. Lamarre, A. Lasenby, C. R. Lawrence, R. Leonardi, P. Leto, P. B. Lilje, M. Linden-Vørnle, M. López-Caniego, J. F. Macías-Pérez, B. Maffei, D. Maino, N. Mandolesi, P. G. Martin, S. Masi, M. Massardi, S. Matarrese, P. Mazzotta, L. Mendes, A. Mennella, M. Migliaccio, M. A. Miville-Deschênes, A. Moneti, L. Montier, G. Morgante, D. Mortlock, D. Munshi, J. A. Murphy, P. Naselsky, F. Nati, P. Natoli, F. Noviello, D. Novikov, I. Novikov, L. Pagano, F. Pajot, R. Paladini, D. Paoletti, M. Peel, O. Perdereau, F. Perrotta, F. Piacentini, M. Piat, D. Pietrobon, S. Plaszczynski, E. Pointecouteau, G. Polenta, L. Popa, G. W. Pratt, P. Procopio, S. Prunet, J. L. Puget, J. P. Rachen, M. Reinecke, M. Remazeilles, S. Ricciardi, T. Riller, I. Ristorcelli, G. Rocha, C. Rosset, G. Roudier, J. A. Rubiño-Martín, B. Rusholme, M. Sandri, G. Savini, D. Scott, L. D. Spencer, V. Stolyarov, D. Sutton, A. S. Suur-Uski, J. F. Sygnet, J. A. Tauber, L. Terenzi, L. Toffolatti, M. Tomasi, C. Trigilio, M. Tristram, T. Trombetti, M. Tucci, G. Umana, J. Valiviita, B. Van Tent, P. Vielva, F. Villa, L. A. Wade, B. D. Wandelt, A. Zacchei, A. Zijlstra, A. Zonca

Physics

Research output: Contribution to journal › Article › peer-review

6 Scopus citations

Abstract

Late stages of stellar evolution are characterized by copious mass-loss events whose signature is the formation of circumstellar envelopes (CSE). Planck multi-frequency measurements have provided relevant information on a sample of Galactic planetary nebulae (PNe) in the important and relatively unexplored observational band between 30 and 857 GHz. Planck enables the assembly of comprehensive PNe spectral energy distributions (SEDs) from radio to far-IR frequencies. Modelling the derived SEDs provides us with information on physical properties of CSEs and the mass content of both main components: ionized gas, traced by the free-free emission at cm-mm waves; and thermal dust, traced by the millimetre and far-IR emission. In particular, the amount of ionized gas and dust has been derived here. Such quantities have also been estimated for the very young PN CRL? 618, where the strong variability observed in its radio and millimetre emission has previously prevented constructing its SED. A morphological study of the Helix Nebula was also performed. Planck maps reveal, for the first time, the spatial distribution of the dust inside the envelope, allowing us to identify different components, the most interesting of which is a very extended component (up to 1? pc) that may be related to a region where the slow expanding envelope is interacting with the surrounding interstellar medium.

Original language	English (US)
Article number	A6
Journal	Astronomy and Astrophysics
Volume	573
DOIs	https://doi.org/10.1051/0004-6361/201423836
State	Published - Jan 1 2015

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Keywords

Planetary nebulae: general
Radio continuum: ISM
Submillimeter: ISM

Access to Document

10.1051/0004-6361/201423836

Cite this

Arnaud, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoit-Lévy, A., Bernard, J. P., Bersanelli, M., Bielewicz, P., Bonaldi, A., Bond, J. R., Borrill, J., Bouchet, F. R., Buemi, C. S., Burigana, C., Cardoso, J. F., ... Zonca, A. (2015). Planck intermediate results XVIII the millimetre and sub-millimetre emission from planetary nebulae. Astronomy and Astrophysics, 573, Article A6. https://doi.org/10.1051/0004-6361/201423836

@article{5063fe2b847945289fdbc61c150b1762,

title = "Planck intermediate results XVIII the millimetre and sub-millimetre emission from planetary nebulae",

abstract = "Late stages of stellar evolution are characterized by copious mass-loss events whose signature is the formation of circumstellar envelopes (CSE). Planck multi-frequency measurements have provided relevant information on a sample of Galactic planetary nebulae (PNe) in the important and relatively unexplored observational band between 30 and 857 GHz. Planck enables the assembly of comprehensive PNe spectral energy distributions (SEDs) from radio to far-IR frequencies. Modelling the derived SEDs provides us with information on physical properties of CSEs and the mass content of both main components: ionized gas, traced by the free-free emission at cm-mm waves; and thermal dust, traced by the millimetre and far-IR emission. In particular, the amount of ionized gas and dust has been derived here. Such quantities have also been estimated for the very young PN CRL? 618, where the strong variability observed in its radio and millimetre emission has previously prevented constructing its SED. A morphological study of the Helix Nebula was also performed. Planck maps reveal, for the first time, the spatial distribution of the dust inside the envelope, allowing us to identify different components, the most interesting of which is a very extended component (up to 1? pc) that may be related to a region where the slow expanding envelope is interacting with the surrounding interstellar medium.",

keywords = "Planetary nebulae: general, Radio continuum: ISM, Submillimeter: ISM",

author = "M. Arnaud and F. Atrio-Barandela and J. Aumont and C. Baccigalupi and Banday, {A. J.} and Barreiro, {R. B.} and E. Battaner and K. Benabed and A. Benoit-L{\'e}vy and Bernard, {J. P.} and M. Bersanelli and P. Bielewicz and A. Bonaldi and Bond, {J. R.} and J. Borrill and Bouchet, {F. R.} and Buemi, {C. S.} and C. Burigana and Cardoso, {J. F.} and S. Casassus and A. Catalano and L. Cerrigone and A. Chamballu and Chiang, {H. C.} and S. Colombi and Colombo, {L. P.L.} and F. Couchot and Crill, {B. P.} and A. Curto and F. Cuttaia and Davies, {R. D.} and Davis, {R. J.} and {De Bernardis}, P. and {De Rosa}, A. and {De Zotti}, G. and J. Delabrouille and C. Dickinson and Diego, {J. M.} and S. Donzelli and O. Dor{\'e} and X. Dupac and En{\ss}lin, {T. A.} and Eriksen, {H. K.} and F. Finelli and M. Frailis and E. Franceschi and S. Galeotta and K. Ganga and M. Giard and J. Gonz{\'a}lez-Nuevo and G{\'o}rski, {K. M.} and A. Gregorio and A. Gruppuso and Hansen, {F. K.} and Harrison, {D. L.} and Hildebrandt, {S. R.} and E. Hivon and Holmes, {W. A.} and Hora, {J. L.} and A. Hornstrup and W. Hovest and Huffenberger, {K. M.} and Jaffe, {T. R.} and Jones, {W. C.} and M. Juvela and E. Keih{\"a}nen and R. Keskitalo and Kisner, {T. S.} and J. Knoche and M. Kunz and H. Kurki-Suonio and A. L{\"a}hteenm{\"a}ki and Lamarre, {J. M.} and A. Lasenby and Lawrence, {C. R.} and R. Leonardi and P. Leto and Lilje, {P. B.} and M. Linden-V{\o}rnle and M. L{\'o}pez-Caniego and Mac{\'i}as-P{\'e}rez, {J. F.} and B. Maffei and D. Maino and N. Mandolesi and Martin, {P. G.} and S. Masi and M. Massardi and S. Matarrese and P. Mazzotta and L. Mendes and A. Mennella and M. Migliaccio and Miville-Desch{\^e}nes, {M. A.} and A. Moneti and L. Montier and G. Morgante and D. Mortlock and D. Munshi and Murphy, {J. A.} and P. Naselsky and F. Nati and P. Natoli and F. Noviello and D. Novikov and I. Novikov and L. Pagano and F. Pajot and R. Paladini and D. Paoletti and M. Peel and O. Perdereau and F. Perrotta and F. Piacentini and M. Piat and D. Pietrobon and S. Plaszczynski and E. Pointecouteau and G. Polenta and L. Popa and Pratt, {G. W.} and P. Procopio and S. Prunet and Puget, {J. L.} and Rachen, {J. P.} and M. Reinecke and M. Remazeilles and S. Ricciardi and T. Riller and I. Ristorcelli and G. Rocha and C. Rosset and G. Roudier and Rubi{\~n}o-Mart{\'i}n, {J. A.} and B. Rusholme and M. Sandri and G. Savini and D. Scott and Spencer, {L. D.} and V. Stolyarov and D. Sutton and Suur-Uski, {A. S.} and Sygnet, {J. F.} and Tauber, {J. A.} and L. Terenzi and L. Toffolatti and M. Tomasi and C. Trigilio and M. Tristram and T. Trombetti and M. Tucci and G. Umana and J. Valiviita and {Van Tent}, B. and P. Vielva and F. Villa and Wade, {L. A.} and Wandelt, {B. D.} and A. Zacchei and A. Zijlstra and A. Zonca",

note = "Funding Information: The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at http://www.sciops.esa.int/index.php?project=planck&page=Planck_Collaboration The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. L. Cerrigone acknowledges funding from the Spanish Consejo Superior de Investigaciones Cient{\'i}ficas through a JAE-Doc research contract, co-funded by the European Social Fund. L. C. thanks the Spanish MICINN for funding support through grants AYA2009-07304 and CSD2009-00038. Publisher Copyright: {\textcopyright} ESO, 2014.",

year = "2015",

month = jan,

day = "1",

doi = "10.1051/0004-6361/201423836",

language = "English (US)",

volume = "573",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

Arnaud, M, Atrio-Barandela, F, Aumont, J, Baccigalupi, C, Banday, AJ, Barreiro, RB, Battaner, E, Benabed, K, Benoit-Lévy, A, Bernard, JP, Bersanelli, M, Bielewicz, P, Bonaldi, A, Bond, JR, Borrill, J, Bouchet, FR, Buemi, CS, Burigana, C, Cardoso, JF, Casassus, S, Catalano, A, Cerrigone, L, Chamballu, A, Chiang, HC, Colombi, S, Colombo, LPL, Couchot, F, Crill, BP, Curto, A, Cuttaia, F, Davies, RD, Davis, RJ, De Bernardis, P, De Rosa, A, De Zotti, G, Delabrouille, J, Dickinson, C, Diego, JM, Donzelli, S, Doré, O, Dupac, X, Enßlin, TA, Eriksen, HK, Finelli, F, Frailis, M, Franceschi, E, Galeotta, S, Ganga, K, Giard, M, González-Nuevo, J, Górski, KM, Gregorio, A, Gruppuso, A, Hansen, FK, Harrison, DL, Hildebrandt, SR, Hivon, E, Holmes, WA, Hora, JL, Hornstrup, A, Hovest, W, Huffenberger, KM, Jaffe, TR, Jones, WC, Juvela, M, Keihänen, E, Keskitalo, R, Kisner, TS, Knoche, J, Kunz, M, Kurki-Suonio, H, Lähteenmäki, A, Lamarre, JM, Lasenby, A, Lawrence, CR, Leonardi, R, Leto, P, Lilje, PB, Linden-Vørnle, M, López-Caniego, M, Macías-Pérez, JF, Maffei, B, Maino, D, Mandolesi, N, Martin, PG, Masi, S, Massardi, M, Matarrese, S, Mazzotta, P, Mendes, L, Mennella, A, Migliaccio, M, Miville-Deschênes, MA, Moneti, A, Montier, L, Morgante, G, Mortlock, D, Munshi, D, Murphy, JA, Naselsky, P, Nati, F, Natoli, P, Noviello, F, Novikov, D, Novikov, I, Pagano, L, Pajot, F, Paladini, R, Paoletti, D, Peel, M, Perdereau, O, Perrotta, F, Piacentini, F, Piat, M, Pietrobon, D, Plaszczynski, S, Pointecouteau, E, Polenta, G, Popa, L, Pratt, GW, Procopio, P, Prunet, S, Puget, JL, Rachen, JP, Reinecke, M, Remazeilles, M, Ricciardi, S, Riller, T, Ristorcelli, I, Rocha, G, Rosset, C, Roudier, G, Rubiño-Martín, JA, Rusholme, B, Sandri, M, Savini, G, Scott, D, Spencer, LD, Stolyarov, V, Sutton, D, Suur-Uski, AS, Sygnet, JF, Tauber, JA, Terenzi, L, Toffolatti, L, Tomasi, M, Trigilio, C, Tristram, M, Trombetti, T, Tucci, M, Umana, G, Valiviita, J, Van Tent, B, Vielva, P, Villa, F, Wade, LA, Wandelt, BD, Zacchei, A, Zijlstra, A & Zonca, A 2015, 'Planck intermediate results XVIII the millimetre and sub-millimetre emission from planetary nebulae', Astronomy and Astrophysics, vol. 573, A6. https://doi.org/10.1051/0004-6361/201423836

TY - JOUR

T1 - Planck intermediate results XVIII the millimetre and sub-millimetre emission from planetary nebulae

AU - Arnaud, M.

AU - Atrio-Barandela, F.

AU - Aumont, J.

AU - Baccigalupi, C.

AU - Banday, A. J.

AU - Barreiro, R. B.

AU - Battaner, E.

AU - Benabed, K.

AU - Benoit-Lévy, A.

AU - Bernard, J. P.

AU - Bersanelli, M.

AU - Bielewicz, P.

AU - Bonaldi, A.

AU - Bond, J. R.

AU - Borrill, J.

AU - Bouchet, F. R.

AU - Buemi, C. S.

AU - Burigana, C.

AU - Cardoso, J. F.

AU - Casassus, S.

AU - Catalano, A.

AU - Cerrigone, L.

AU - Chamballu, A.

AU - Chiang, H. C.

AU - Colombi, S.

AU - Colombo, L. P.L.

AU - Couchot, F.

AU - Crill, B. P.

AU - Curto, A.

AU - Cuttaia, F.

AU - Davies, R. D.

AU - Davis, R. J.

AU - De Bernardis, P.

AU - De Rosa, A.

AU - De Zotti, G.

AU - Delabrouille, J.

AU - Dickinson, C.

AU - Diego, J. M.

AU - Donzelli, S.

AU - Doré, O.

AU - Dupac, X.

AU - Enßlin, T. A.

AU - Eriksen, H. K.

AU - Finelli, F.

AU - Frailis, M.

AU - Franceschi, E.

AU - Galeotta, S.

AU - Ganga, K.

AU - Giard, M.

AU - González-Nuevo, J.

AU - Górski, K. M.

AU - Gregorio, A.

AU - Gruppuso, A.

AU - Hansen, F. K.

AU - Harrison, D. L.

AU - Hildebrandt, S. R.

AU - Hivon, E.

AU - Holmes, W. A.

AU - Hora, J. L.

AU - Hornstrup, A.

AU - Hovest, W.

AU - Huffenberger, K. M.

AU - Jaffe, T. R.

AU - Jones, W. C.

AU - Juvela, M.

AU - Keihänen, E.

AU - Keskitalo, R.

AU - Kisner, T. S.

AU - Knoche, J.

AU - Kunz, M.

AU - Kurki-Suonio, H.

AU - Lähteenmäki, A.

AU - Lamarre, J. M.

AU - Lasenby, A.

AU - Lawrence, C. R.

AU - Leonardi, R.

AU - Leto, P.

AU - Lilje, P. B.

AU - Linden-Vørnle, M.

AU - López-Caniego, M.

AU - Macías-Pérez, J. F.

AU - Maffei, B.

AU - Maino, D.

AU - Mandolesi, N.

AU - Martin, P. G.

AU - Masi, S.

AU - Massardi, M.

AU - Matarrese, S.

AU - Mazzotta, P.

AU - Mendes, L.

AU - Mennella, A.

AU - Migliaccio, M.

AU - Miville-Deschênes, M. A.

AU - Moneti, A.

AU - Montier, L.

AU - Morgante, G.

AU - Mortlock, D.

AU - Munshi, D.

AU - Murphy, J. A.

AU - Naselsky, P.

AU - Nati, F.

AU - Natoli, P.

AU - Noviello, F.

AU - Novikov, D.

AU - Novikov, I.

AU - Pagano, L.

AU - Pajot, F.

AU - Paladini, R.

AU - Paoletti, D.

AU - Peel, M.

AU - Perdereau, O.

AU - Perrotta, F.

AU - Piacentini, F.

AU - Piat, M.

AU - Pietrobon, D.

AU - Plaszczynski, S.

AU - Pointecouteau, E.

AU - Polenta, G.

AU - Popa, L.

AU - Pratt, G. W.

AU - Procopio, P.

AU - Prunet, S.

AU - Puget, J. L.

AU - Rachen, J. P.

AU - Reinecke, M.

AU - Remazeilles, M.

AU - Ricciardi, S.

AU - Riller, T.

AU - Ristorcelli, I.

AU - Rocha, G.

AU - Rosset, C.

AU - Roudier, G.

AU - Rubiño-Martín, J. A.

AU - Rusholme, B.

AU - Sandri, M.

AU - Savini, G.

AU - Scott, D.

AU - Spencer, L. D.

AU - Stolyarov, V.

AU - Sutton, D.

AU - Suur-Uski, A. S.

AU - Sygnet, J. F.

AU - Tauber, J. A.

AU - Terenzi, L.

AU - Toffolatti, L.

AU - Tomasi, M.

AU - Trigilio, C.

AU - Tristram, M.

AU - Trombetti, T.

AU - Tucci, M.

AU - Umana, G.

AU - Valiviita, J.

AU - Van Tent, B.

AU - Vielva, P.

AU - Villa, F.

AU - Wade, L. A.

AU - Wandelt, B. D.

AU - Zacchei, A.

AU - Zijlstra, A.

AU - Zonca, A.

N1 - Funding Information: The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at http://www.sciops.esa.int/index.php?project=planck&page=Planck_Collaboration The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. L. Cerrigone acknowledges funding from the Spanish Consejo Superior de Investigaciones Científicas through a JAE-Doc research contract, co-funded by the European Social Fund. L. C. thanks the Spanish MICINN for funding support through grants AYA2009-07304 and CSD2009-00038. Publisher Copyright: © ESO, 2014.

PY - 2015/1/1

Y1 - 2015/1/1

N2 - Late stages of stellar evolution are characterized by copious mass-loss events whose signature is the formation of circumstellar envelopes (CSE). Planck multi-frequency measurements have provided relevant information on a sample of Galactic planetary nebulae (PNe) in the important and relatively unexplored observational band between 30 and 857 GHz. Planck enables the assembly of comprehensive PNe spectral energy distributions (SEDs) from radio to far-IR frequencies. Modelling the derived SEDs provides us with information on physical properties of CSEs and the mass content of both main components: ionized gas, traced by the free-free emission at cm-mm waves; and thermal dust, traced by the millimetre and far-IR emission. In particular, the amount of ionized gas and dust has been derived here. Such quantities have also been estimated for the very young PN CRL? 618, where the strong variability observed in its radio and millimetre emission has previously prevented constructing its SED. A morphological study of the Helix Nebula was also performed. Planck maps reveal, for the first time, the spatial distribution of the dust inside the envelope, allowing us to identify different components, the most interesting of which is a very extended component (up to 1? pc) that may be related to a region where the slow expanding envelope is interacting with the surrounding interstellar medium.

AB - Late stages of stellar evolution are characterized by copious mass-loss events whose signature is the formation of circumstellar envelopes (CSE). Planck multi-frequency measurements have provided relevant information on a sample of Galactic planetary nebulae (PNe) in the important and relatively unexplored observational band between 30 and 857 GHz. Planck enables the assembly of comprehensive PNe spectral energy distributions (SEDs) from radio to far-IR frequencies. Modelling the derived SEDs provides us with information on physical properties of CSEs and the mass content of both main components: ionized gas, traced by the free-free emission at cm-mm waves; and thermal dust, traced by the millimetre and far-IR emission. In particular, the amount of ionized gas and dust has been derived here. Such quantities have also been estimated for the very young PN CRL? 618, where the strong variability observed in its radio and millimetre emission has previously prevented constructing its SED. A morphological study of the Helix Nebula was also performed. Planck maps reveal, for the first time, the spatial distribution of the dust inside the envelope, allowing us to identify different components, the most interesting of which is a very extended component (up to 1? pc) that may be related to a region where the slow expanding envelope is interacting with the surrounding interstellar medium.

KW - Planetary nebulae: general

KW - Radio continuum: ISM

KW - Submillimeter: ISM

UR - http://www.scopus.com/inward/record.url?scp=84916623092&partnerID=8YFLogxK

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U2 - 10.1051/0004-6361/201423836

DO - 10.1051/0004-6361/201423836

M3 - Article

AN - SCOPUS:84916623092

SN - 0004-6361

VL - 573

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

M1 - A6

ER -

Planck intermediate results XVIII the millimetre and sub-millimetre emission from planetary nebulae

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