Absorption Line Signatures of Delayed Dwarfs

Details Absorption Line Signatures of Delayed Dwarfs Absorption Line Signatures of Delayed Dwarfs

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aas...191.8409k&link_type=abstract

American Astronomical Society, 191st AAS Meeting, #84.09; Bulletin of the American Astronomical Society, Vol. 29, p.1350

Astronomy and Astrophysics

Astronomy

Scientific paper

Recent theoretical work suggests that the UV background may delay the epoch at which gas in small dark matter halos can cool and form stars. We compute the UV absorption line signatures of these objects and discuss their detectability by the STIS and FUSE instruments. In addition, we discuss the potential correspondence of delayed dwarfs with observed systems where no optical counterpart is seen.

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