| dc.contributor.author | BALMAN, Şölen | |
| dc.date.accessioned | 2021-03-03T09:18:34Z | |
| dc.date.available | 2021-03-03T09:18:34Z | |
| dc.identifier.citation | BALMAN Ş., "Pre-outburst Chandra observations of the recurrent nova T Pyxidis", ASTRONOMY & ASTROPHYSICS, cilt.572, 2014 | |
| dc.identifier.issn | 0004-6361 | |
| dc.identifier.other | vv_1032021 | |
| dc.identifier.other | av_1c4ec3f8-0b53-4d08-b7bc-edde08372075 | |
| dc.identifier.uri | http://hdl.handle.net/20.500.12627/24273 | |
| dc.identifier.uri | https://doi.org/10.1051/0004-6361/201424233 | |
| dc.description.abstract | Aims. I study the spectral, temporal, and spatial characteristics of the quiescent X-ray emission (not in outburst) of the recurrent nova T Pyx. | |
| 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 | Pre-outburst Chandra observations of the recurrent nova T Pyxidis | |
| dc.type | Makale | |
| dc.relation.journal | ASTRONOMY & ASTROPHYSICS | |
| dc.contributor.department | , , | |
| dc.identifier.volume | 572 | |
| dc.contributor.firstauthorID | 2211733 | |
