Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 28
... clouds is presented by Shu et al . ( 1987 ) : here we are concerned only with the formation of massive stars in such clouds . How is the mass spectrum of these stars ( IMF ) related to the initial properties of the clouds such as ...
... clouds is presented by Shu et al . ( 1987 ) : here we are concerned only with the formation of massive stars in such clouds . How is the mass spectrum of these stars ( IMF ) related to the initial properties of the clouds such as ...
Page 29
... cloud . A good review is presented by Elmegreen ( 1986 ) . 3.1 Molecular Clouds While a substantial portion of interstellar molecular gas is thought to be contained in dwarf clouds that are not restricted to spiral arms , it is the giant ...
... cloud . A good review is presented by Elmegreen ( 1986 ) . 3.1 Molecular Clouds While a substantial portion of interstellar molecular gas is thought to be contained in dwarf clouds that are not restricted to spiral arms , it is the giant ...
Page 31
... cloud . A good review is presented by Elmegreen ( 1986 ) . 3.1 Molecular Clouds While a substantial portion of interstellar molecular gas is thought to be contained in dwarf clouds that are not restricted to spiral arms , it is the giant ...
... cloud . A good review is presented by Elmegreen ( 1986 ) . 3.1 Molecular Clouds While a substantial portion of interstellar molecular gas is thought to be contained in dwarf clouds that are not restricted to spiral arms , it is the giant ...
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abundance additional analysis appear associations assumed Astronomical average binary blue bright calibration catalog central clouds cluster color compared correction derived detection determined discussed distance distribution dwarf eclipse effects emission errors estimate et al evidence evolution field Figure flux frame function galaxies giants given groups included increase indices less light limit lines luminosity magnitude mass mean measured MNRAS nebulae noted objects observations obtained optical orbital PASP period phase photometric pixels position possible present probably quasars range ratio reduced reference region relation relative rotation sample scale scatter secondary shown similar sources spectral spectrum standard stars stellar stellar winds suggests surface survey Table telescope temperature tion University values variability velocity wavelength X-ray