The first definitive binary orbit determined with the Hubble Space Telescope fine guidance sensors: Wolf 1062 (Gliese 748)

Astronomical Journal

Volumn 116, Issue 3, 1998, Pages 1432-1439

  Franz, Otto G ^a   Henry, Todd J ^b   Wasserman, Lawrence H ^a   Benedict, G Fritz ^c   Ianna, Philip A ^d   Kirkpatrick, J Davy ^e   McCarthy Jr , Donald W ^f   Bradley, Arthur J ^g   Duncombe, Raynor L ^h   Fredrick, Laurence W ^d   Hemenway, Paul D ⁱ   Jefferys, William H ^c   McArthur, Barbara E ^c   Nelan, Edmund P ^j   Shelus, Peter J ^c   Story, Darrell B ^k   Van Altena, William F ^l   Whipple, Arthur L ^g  

^a LOWELL OBSERVATORY   (United States)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c UNIVERSITY OF TEXAS AT AUSTIN   (United States)

^d UNIVERSITY OF VIRGINIA   (United States)

^e CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^f UNIVERSITY OF ARIZONA   (United States)

^g HONEYWELL   (United States)

^h The University of Texas at Austin   (United States)

ⁱ UNIVERSITY OF RHODE ISLAND   (United States)

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

^k Jackson and Tull   (United States)

^l YALE UNIVERSITY   (United States)

more..

Author keywords

Astrometry binaries; Close stars; Fundamental parameters stars; Individual (Wolf 1062) stars; Low mass, brown dwarfs

Indexed keywords

EID: 17444444958     PISSN: 00046256     EISSN: None     Source Type: Journal    
DOI: 10.1086/300500     Document Type: Article

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