Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2297
Full metadata record
DC FieldValueLanguage
dc.contributor.authorManchanda, R. K-
dc.date.accessioned2008-05-13T11:43:19Z-
dc.date.available2008-05-13T11:43:19Z-
dc.date.issued2001-
dc.identifier.citationBASI, Vol. 29, No. 3, pp. 429 - 433en
dc.identifier.urihttp://hdl.handle.net/2248/2297-
dc.description.abstractWe report spectral measurements of the bright QSO 3C273 and the AGN source NGC 5506 made during a balloon flight experiment using high sensitivity scintillation counter telescope LASE, operating in the 20-200 keV energy band. The observations were made on Nov. 20, 1998 from Hyderabad, S. India. The observed spectrum for 3C 273 and is best fitted with a power law of the form = KE-? and the measure luminosity compares with earlier measurements by SIGMA and OSSE satellites. The observed spectra of NGC 5506 was found to be very hard although the total luminosity was much lower than the earlier observations and is consistent with the time variability of the AGN sources, Spectral data is discussed in terms of non-thermal emission models and X-ray emission geometry.en
dc.format.extent361629 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2001BASI...29..429Men
dc.subjectX-ray emissionen
dc.subjectExtragalacticen
dc.subjectAGNen
dc.subjectNGC 5506en
dc.titleObservation of hard X-ray emission from extragalactic sources 3C 273 and NGC 5506 in 20-200 keV banden
dc.typeArticleen
Appears in Collections:BASI Publications

Files in This Item:
File Description SizeFormat 
Manch.pdf353.15 kBAdobe PDFView/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.