Chandra astrometry sets a tight upper limit to the proper motion of SGR 1900+14

Astrophysical Journal

Volumn 692, Issue 1, 2009, Pages 158-161

  De Luca, A ^a,b,d   Caraveo, P A ^a   Esposito, P ^a,c,d   Hurley, K ^e  

^a INAF IASF MILANO   (Italy)

^b SCUOLA UNIVERSITARIA SUPERIORE IUSS PAVIA   (Italy)

^c UNIVERSITY OF PAVIA   (Italy)

^d INFN SEZIONE DI PAVIA   (Italy)

^e UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

stars: neutron; supernova remnants; X rays: stars

Indexed keywords

EID: 66649099215     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/692/1/158     Document Type: Article

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