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dc.contributor.authorYoldas, AK
dc.contributor.authorBALMAN, Şölen
dc.date.accessioned2021-03-05T19:26:08Z
dc.date.available2021-03-05T19:26:08Z
dc.date.issued2002
dc.identifier.citationYoldas A., BALMAN Ş., "CHANDRA detection of 16 new X-ray sources", ASTRONOMY & ASTROPHYSICS, cilt.384, ss.190-194, 2002
dc.identifier.issn1432-0746
dc.identifier.otherav_cf4c2f76-7c8a-4d01-9ea7-5951659c073b
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/137074
dc.identifier.urihttps://doi.org/10.1051/0004-6361:20011837
dc.description.abstractWe have detected 18 sources over 6sigma threshold within two regions 8'.3 x 16'.9 and 8'.3 x 33'.6 in the vicinity of the point with alpha = 03(h)31(m)02.(s)45 (J2000) and delta = +43degrees47'58".5 (J2000) using a CHANDRA ACIS (S+I) observation. Two of the sources were detected before with ROSAT HRI and one source could be closely identified with a star in the optical catalog, USNO A-2. We have also studied source spectra applying four spectral models to the data. Most of the sources can be classified as Cataclysmic Variable, Low Mass X-ray Binary or single star candidates due to their spectral characteristics and luminosities. We also searched for the extragalactic origin for these 18 sources. The source count rates vary between 5.8x10(-4) -4.7x10(-3) counts/s. Due to low count rates temporal characteristics of the sources can not be studied effectively.
dc.language.isoeng
dc.subjectTemel Bilimler (SCI)
dc.subjectAstronomi ve Astrofizik
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectUzay bilimi
dc.subjectFizik
dc.subjectTemel Bilimler
dc.titleCHANDRA detection of 16 new X-ray sources
dc.typeMakale
dc.relation.journalASTRONOMY & ASTROPHYSICS
dc.contributor.department, ,
dc.identifier.volume384
dc.identifier.issue1
dc.identifier.startpage190
dc.identifier.endpage194
dc.contributor.firstauthorID2212670


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