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Two-phase spectrum of the black hole candidate 1E1740.7-2942
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Faculty of Science and Technology, Astronomical observatory.
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1998 (English)In: PHYSICA SCRIPTA, ISSN 0281-1847, Vol. T77, 86-87 p.Article in journal (Refereed) Published
Abstract [en]

Combined ASCA and SIGMA data of 1E1740.7-2942 during its standard state (September 1993 and 1994) were successfully fitted with a two-phase model ISM (iterative scattering method) [1]. The classical cold accretion disk does not extend up to the innermost

Place, publisher, year, edition, pages
ROYAL SWEDISH ACAD SCIENCES , 1998. Vol. T77, 86-87 p.
Keyword [en]
X-RAY; MOLECULAR CLOUD; 1E-1740.7-2942; GINGA
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:uu:diva-85287OAI: oai:DiVA.org:uu-85287DiVA: diva2:113195
Note
Addresses: Nevalainen J, Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 01238 USA. Harvard Smithsonian Ctr Astrophys, Cambridge, MA 01238 USA. Univ Helsinki, FIN-00014 Helsinki, Finland. Astron Observ, SE-75120 Uppsala, Sweden. NORDITA, DKAvailable from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-14

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