| dc.contributor.author | ORIO, M | |
| dc.contributor.author | OGELMAN, H | |
| dc.contributor.author | BALMAN, Şölen | |
| dc.date.accessioned | 2021-03-06T21:12:50Z | |
| dc.date.available | 2021-03-06T21:12:50Z | |
| dc.date.issued | 1995 | |
| dc.identifier.citation | BALMAN Ş., ORIO M., OGELMAN H., "ROSAT OBSERVATION OF THE OLD CLASSICAL NOVA CP PUPPIS", ASTROPHYSICAL JOURNAL, cilt.449, 1995 | |
| dc.identifier.issn | 0004-637X | |
| dc.identifier.other | vv_1032021 | |
| dc.identifier.other | av_fdac6fe1-12b6-46ef-bc81-a663199b21b3 | |
| dc.identifier.uri | http://hdl.handle.net/20.500.12627/165935 | |
| dc.identifier.uri | https://doi.org/10.1086/309628 | |
| dc.description.abstract | We present X-ray observation of the old nova CP Puppis obtained by the ROSAT Position Sensitive Proportional Counter in 1993 April. The source is detected with a count rate of 0.067 +/- 0.004 counts s(-1). The total observed X-ray flux between 0.1 and 2.4 keV is similar to 3 X 10(-12) ergs s(-1) cm(-2). The spectrum of the source is best fit by a thermal bremsstrahlung emission model with temperature greater than or equal to 1 keV. The X-ray count rates are modulated with the previously known spectroscopic period similar to 0(d).0614 ( similar to 88.4 minutes) of the system at the 3 sigma confidence level. The hard X-ray flux and the detected X-ray modulations suggest that CP Puppis is an intermediate polar system. | |
| dc.language.iso | eng | |
| dc.subject | Astronomi ve Astrofizik | |
| dc.subject | Temel Bilimler | |
| dc.subject | Fizik | |
| dc.subject | Temel Bilimler (SCI) | |
| dc.subject | Uzay bilimi | |
| dc.subject | ASTRONOMİ VE ASTROFİZİK | |
| dc.title | ROSAT OBSERVATION OF THE OLD CLASSICAL NOVA CP PUPPIS | |
| dc.type | Makale | |
| dc.relation.journal | ASTROPHYSICAL JOURNAL | |
| dc.contributor.department | , , | |
| dc.identifier.volume | 449 | |
| dc.identifier.issue | 1 | |
| dc.contributor.firstauthorID | 2212686 | |
