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Astronomical Journal

Volumn 143, Issue 6, 2012, Pages

Converting from 3.6 and 4.5μm fluxes to stellar mass

(3) Eskew, Michael a,b Zaritsky, Dennis b Meidt, Sharon c

a The University of Texas at Austin (United States)

b UNIVERSITY OF ARIZONA (United States)

c MAX PLANCK INSTITUT FÜR ASTRONOMIE (Germany)

Author keywords

galaxies: fundamental parameters; galaxies: stellar content; Magellanic Clouds

Indexed keywords

EID: 84862066125 PISSN: 00046256 EISSN: None Source Type: Journal
DOI: 10.1088/0004-6256/143/6/139 Document Type: Article

Times cited : (42)

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