dc.contributor.author |
Revnivtsev M. |
|
dc.contributor.author |
Lutovinov A. |
|
dc.contributor.author |
Suleimanov V. |
|
dc.contributor.author |
Sunyaev R. |
|
dc.contributor.author |
Zheleznyakov V. |
|
dc.date.accessioned |
2018-09-17T20:07:09Z |
|
dc.date.available |
2018-09-17T20:07:09Z |
|
dc.date.issued |
2004 |
|
dc.identifier.issn |
0004-6361 |
|
dc.identifier.uri |
https://dspace.kpfu.ru/xmlui/handle/net/133061 |
|
dc.description.abstract |
We present the broadband phase averaged spectrum of one of the brightest intermediate polars V1223 Sgr, obtained with INTEGRAL and RXTE observatories (3-100 keV). Good statistical quality of the spectrum in a hard X-ray energy band (INTEGRAL/IBIS and RXTE/HEXTE) allowed us to disentangle contributions of a direct optically thin plasma emission and a reflected component to the spectrum of V1223 Sgr. The obtained measurement of the post-shock temperature of the accreting matter give us the information about the mass of the white dwarf and the inclination of the system. |
|
dc.relation.ispartofseries |
Astronomy and Astrophysics |
|
dc.subject |
Stars: binaries: general |
|
dc.subject |
Stars: individual: V1223 Sgr |
|
dc.subject |
X-rays: binaries |
|
dc.title |
Broadband X-ray spectrum of intermediate polar V1223 Sgr |
|
dc.type |
Article |
|
dc.relation.ispartofseries-issue |
1 |
|
dc.relation.ispartofseries-volume |
426 |
|
dc.collection |
Публикации сотрудников КФУ |
|
dc.relation.startpage |
253 |
|
dc.source.id |
SCOPUS00046361-2004-426-1-SID6344240730 |
|