Ages for globular clusters in the outer galactic halo: The second-parameter clusters Palomar 3, Palomar 4, and Eridanus

Astronomical Journal

Volumn 117, Issue 1, 1999, Pages 247-263

  Stetson, Peter B ^a   Bolte, Michael ^b   Harris, William E ^c   Hesser, James E ^a   Van Den Bergh, Sidney ^a   Vandenberg, Don A ^d   Bell, Roger A ^e   Johnson, Jennifer A ^b   Bond, Howard E ^f   Fullton, Laura K ^f   Fahlman, Gregory G ^g   Richer, Harvey B ^g  

^a NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^b University of California at Santa Cruz   (United States)

^c MCMASTER UNIVERSITY   (Canada)

^d UNIVERSITY OF VICTORIA   (Canada)

^e UNIVERSITY OF MARYLAND   (United States)

^f AURA for the European Space Agency   (United States)

^g UNIVERSITY OF BRITISH COLUMBIA   (Canada)

Author keywords

Galaxy: formation; Globular clusters: individual (Palomar 3, Palomar 4, Eridanus)

Indexed keywords

EID: 0344923880     PISSN: 00046256     EISSN: None     Source Type: Journal    
DOI: 10.1086/300670     Document Type: Article

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