Zobrazeno 1 - 10
of 20
pro vyhledávání: '"X-rays : stars [stars]"'
Publikováno v:
Acta Polytechnica, Vol 51, Iss 1 (2011)
We present a detailed spectral and timing analysis of the High Mass X-ray Binary (HMXB) 4U 1909+07 with INTEGRAL and RXTE. 4U1909+07 is a persistent accreting X-ray pulsar with a period of approximately 605 s. The period changes erratically consisten
Externí odkaz:
https://doaj.org/article/83c1d04feedf40e09798376b47ca2fa4
Akademický článek
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Autor:
Paul, Biswajit, Raichur, H.
Publikováno v:
宇宙航空研究開発機構特別資料 = JAXA Special Publication: Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop. :102-107
Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop (RIKEN, 10-12 June 2008)
We have carried out detailed investigations of the long term X-ray flux variations of the high mass X-ray binary pulsar Cen X-3 using archival
We have carried out detailed investigations of the long term X-ray flux variations of the high mass X-ray binary pulsar Cen X-3 using archival
Autor:
Luciano Burderi, Alessandro Papitto, R. Iaria, N. R. Robba, Alessandro Riggio, Antonino D'Ai, T. Di Salvo
Recent studies of the optical/UV and X-ray ephemerides of X1822-371 have found some discrepancies in the value of the orbital period derivative. Because of the importance of this value in constraining the system evolution, we comprehensively analyse
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0f943acaf06c6b06b9bfe2b26be0e033
http://hdl.handle.net/10447/61879
http://hdl.handle.net/10447/61879
Autor:
Arvind Parmar, Luigi Stella, F. Frontera, M. van der Klis, Eliana Palazzi, Mauro Orlandini, Lorenzo Amati, Shuang-Nan Zhang, C. Guidorzi, Ruben Farinelli, N. Masetti
Publikováno v:
Scopus-Elsevier
402 (2003): 1021–1032.
info:cnr-pdr/source/autori:Farinelli R., Frontera F., Masetti N., Amati L., Guidorzi C., Orlandini M., Palazzi E., Parmar A.N., Stella L., Van der Klis M., Zhang S.N./titolo:BeppoSAX observations of two unclassified LMXBs: X1543-624 and X1556-605/doi:/rivista:/anno:2003/pagina_da:1021/pagina_a:1032/intervallo_pagine:1021–1032/volume:402
Astronomy & Astrophysics, 402, 1021-1032. EDP Sciences
402 (2003): 1021–1032.
info:cnr-pdr/source/autori:Farinelli R., Frontera F., Masetti N., Amati L., Guidorzi C., Orlandini M., Palazzi E., Parmar A.N., Stella L., Van der Klis M., Zhang S.N./titolo:BeppoSAX observations of two unclassified LMXBs: X1543-624 and X1556-605/doi:/rivista:/anno:2003/pagina_da:1021/pagina_a:1032/intervallo_pagine:1021–1032/volume:402
Astronomy & Astrophysics, 402, 1021-1032. EDP Sciences
Observations of two unclassified Low Mass X-ray Binaries, X1543-624 and X1556-605, are presented. In the 2-10 keV band the first of the two sources is a factor two stronger than the other. Both sources do not show X-ray bursts, dips or eclipses in th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5746774accb0b77ae380c193b6f21c03
Autor:
Moira Jardine, F. M. Walter, J.-F. Donati, Scott G. Gregory, G. A. J. Hussain, Costanza Argiroffi, M. B. Skelly, Jerome Bouvier, Ettore Flaccomio, Konstantin V. Getman
Publikováno v:
NASA Astrophysics Data System
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2011, 530, ⟨10.1051/0004-6361/201016321⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2011, 530, ⟨10.1051/0004-6361/201016321⟩
The soft X-ray emission from high density plasma in CTTS is associated with the accretion process. It is still unclear whether this high density cool plasma is heated in the accretion shock, or if it is coronal plasma fed/modified by the accretion pr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9ce051e5d6087a41eddc2fea6ee9757c
https://resolver.caltech.edu/CaltechAUTHORS:20110610-121129141
https://resolver.caltech.edu/CaltechAUTHORS:20110610-121129141
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 411 (3)
Monthly Notices of the Royal Astronomical Society, 411 (3)
ISSN:0035-8711
ISSN:1365-2966
ISSN:1365-8711
ISSN:0035-8711
ISSN:1365-2966
ISSN:1365-8711
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ff65463f81ee428b0f576844efaaa896
https://hdl.handle.net/20.500.11850/31418
https://hdl.handle.net/20.500.11850/31418
Autor:
Katja Pottschmidt, Laura Barragan, I. Kreykenbohm, Jörn Wilms, Slawomir Suchy, R. E. Rothschild, F. Fürst
Publikováno v:
Joern Wilms
Acta Polytechnica, Vol 51, Iss 1 (2011)
NASA Astrophysics Data System
Acta Polytechnica, Vol 51, Iss 1 (2011)
NASA Astrophysics Data System
We present a detailed spectral and timing analysis of the High Mass X-ray Binary (HMXB) 4U 1909+07 with INTEGRAL and RXTE. 4U1909+07 is a persistent accreting X-ray pulsar with a period of approximately 605 s. The period changes erratically consisten
X-ray flares on the UV Ceti-type star CC Eridani: a 'peculiar' time-evolution of spectral parameters
Autor:
Fabio Reale, Javier Lopez-Santiago, Giuseppina Micela, M. Caramazza, I. Crespo-Chacón, Ignazio Pillitteri
Context: Weak flares are supposed to be an important heating agent of the outer layers of stellar atmospheres. However, due to instrumental limitations, only large X-ray flares have been studied in detail until now. Aims: We used an XMM-Newton observ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b1cbf0096aeee5f9091599a1fa79ca76
http://arxiv.org/abs/0706.3332
http://arxiv.org/abs/0706.3332
Autor:
Fabio Reale
The diagnostics of stellar flaring coronal loops have been so far largely based on the analysis of the decay phase. We derive new diagnostics from the analysis of the rise and peak phase of stellar flares. We release the assumption of full equilibriu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::31476a5e3fcb29eed3ed78757d71bea1