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GALAXY program

We have used the infra-red triplet (921.286 nm, 922.809 nm and 923.754 nm) to determine the sulphur abundance in the 32 giants from ESO s Large Program Galaxy Formation, Early Nucleosynthesis, and First Stars . [Pg.128]

As part of a program to determine the near-IR photometric and spectroscopic properties of bright IRAS galaxies, we have obtained JHK images and medium resolution (A/AA 330) JT-band spectra of VV114. [Pg.125]

Abstract. We present the first results of an IR imaging program to study galaxy erolntion in moderate redshift galaxy dusters. [Pg.155]

SPIREX is part of a larger program to exploit the properties of the South Pole for astrophysical research. It is one of several experimental programs within the Center for Astrophysical Research in Antarctica, or CARA for short. Scientifically, these projects are united by the common goal to understand the origins of the structures in the Universe from stars and galaxies on... [Pg.248]

As part of a program to determine the excitation conditions of the gas and to characterize the stellar population in M82, we have observed this starburst galaxy in the near-in ared, concentrating on the H2 1-0 S(l) line at 2.122/tm, the Br7 emission feature at 2.166 fjoa, and the CO absorption band at 2.35 fim. [Pg.509]

See other pages where GALAXY program is mentioned: [Pg.11]    [Pg.108]    [Pg.259]    [Pg.227]    [Pg.40]    [Pg.246]    [Pg.177]    [Pg.224]    [Pg.259]    [Pg.350]    [Pg.122]    [Pg.273]    [Pg.3]    [Pg.453]    [Pg.23]    [Pg.43]    [Pg.26]    [Pg.85]    [Pg.694]    [Pg.62]    [Pg.145]    [Pg.24]    [Pg.26]    [Pg.101]    [Pg.130]    [Pg.141]    [Pg.148]    [Pg.153]    [Pg.153]    [Pg.315]    [Pg.504]    [Pg.535]    [Pg.627]   
See also in sourсe #XX -- [ Pg.259 ]

See also in sourсe #XX -- [ Pg.259 ]



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Galaxie

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