The Absorption Signatures of Dwarf Galaxies: Thez = 1.04 Multicloud Weak MgiiAbsorber toward PG 1634+706
نویسندگان
چکیده
منابع مشابه
Absorption Line Signatures of Proto-Dwarf Galaxies
SiIV Introduction A substantial fraction of the Ly clouds may be due to gas in small halos corresponding to dwarf galaxies or their progenitors. At low redshifts, for example, van Gorkom et al (1996) have identified a dwarf galaxy fainter than the SMC associated with a Ly cloud detected in the spectrum of Mrk 335. Many of the recent studies of the relationship between Ly clouds and galaxies hav...
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ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 2004
ISSN: 0004-637X,1538-4357
DOI: 10.1086/382939