THE absence of radio emission from the globular cluster G1

Astrophysical Journal Letters

Volumn 755, Issue 1, 2012, Pages

  Miller Jones, J C A ^a   Wrobel, J M ^b   Sivakoff, G R ^c   Heinke, C O ^c   Miller, R E ^c   Plotkin, R M ^d   Di Stefano, R ^e   Greene, J E ^f   Ho, L C ^g   Joseph, T D ^h   Kong, A K H ⁱ   MacCarone, T J ^h  

^a CURTIN UNIVERSITY   (Australia)

^b NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

^c UNIVERSITY OF ALBERTA   (Canada)

^d UNIVERSITY OF AMSTERDAM   (Netherlands)

^e HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

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

^g CARNEGIE OBSERVATORIES   (United States)

^h UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

ⁱ NATIONAL TSING HUA UNIVERSITY   (Taiwan)

Author keywords

accretion; accretion disks; globular clusters: individual (Mayall II = G1); X rays: binaries

Indexed keywords

EID: 84864449135     PISSN: 20418205     EISSN: 20418213     Source Type: Journal    
DOI: 10.1088/2041-8205/755/1/L1     Document Type: Article

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