Lensing of stars by spherical gas clouds

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Abstract

Cold gas clouds of ∼Jovian mass and ∼AU size will act as lenses for optical light. If the Galaxy contains ∼1011M in such clouds, background stars will be magnified at a detectable rate. The resulting light curves can resemble those due to gravitational lensing by a point mass, raising the possibility that some events attributed to gravitational lensing might instead be due to "gaseous lensing." During a lensing event, the lens would impose narrow infrared and far-red H2 absorption lines on the stellar spectrum. Existing programs to observe gravitational microlensing, supplemented by spectroscopy, can therefore be used to either detect such events or place limits on the number of such gas clouds present in the Galaxy.

Original languageEnglish (US)
Pages (from-to)L41-L44
JournalAstrophysical Journal
Volume509
Issue number1 PART II
DOIs
StatePublished - 1998

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Galaxies: ISM
  • Galaxies: halos
  • Galaxy: halo
  • ISM: clouds
  • ISM: molecules

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