Detection of a large Be circumstellar disk during X-ray quiescence of XTE J1946+274

Download

Date

2015-10-01

Author

Arabaci, M. Ozbey
Camero-Arranz, A.
Zurita, C.
Gutierrez-Soto, J.
Nespoli, E.
Suso, J.
Kiaeerad, F.
Garcia-Rojas, J.
Kiziloglu, U.

Metadata

Show full item record

This work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.

Item Usage Stats

108
views

0
downloads

Aims. We present a multiwavelength study of the Be/X-ray binary system XTE J1946+274 with the main goal of better characterizing its behavior during X-ray quiescence. We also aim to shed light on the possible mechanisms which trigger the X-ray activity for this source.

Subject Keywords

Accretion, accretion disks, Stars : emission-line, Be, X-rays: binaries, Pulsars: individual: XTE J1946+274

URI

https://hdl.handle.net/11511/68513

Journal

ASTRONOMY & ASTROPHYSICS

DOI

https://doi.org/10.1051/0004-6361/201425488

Collections

Department of Physics, Article

Suggestions

OpenMETU
Core

X-ray variations in the inner accretion flow of dwarf novae Balman, Şölen; Revnivtsev, M. (2012-10-01) Aims. We study the inner disk structure of dwarf novae (DNe; i.e., nonmagnetic cataclysmic variables).
Reanalysis of high-resolution XMM-Newton data of V2491 Cygni using models of collisionally ionized hot absorbers Balman, Şölen; Gamsizkan, C. (2017-02-01) Aims. We model spectral absorption features in data of the high-resolution XMM-Newton Reflection Grating Spectrometer.
An optical search for supernova remnants in the nearby spiral galaxy NGC 2903 SONBAŞ, EDA; AKYÜZ, AYSUN; Balman, Şölen (EDP Sciences, 2009-01-01) Aims. We present the results of an optical search for supernova remnants (SNRs) in the nearby spiral galaxy NGC 2903.
Effects of pretreated beet molasses on benzaldehyde lyase production by recombinant Escherichia coli BL21(DE3)pLySs Çalık, Pınar (Wiley, 2009-11-01) Aims:
The outburst of Nova CSS 081007:030559+054715 (HV Ceti) Beardmore, A. P.; Osborne, J. P.; Page, K. L.; Hakala, P. J.; Schwarz, G. J.; Rauch, T.; Balman, Şölen; Evans, P. A.; Goad, M. R.; Ness, J. -U.; Starrfield, S.; Wagner, R. M. (2012-09-01) Aims. The outburst of nova CSS 081007:030559+054715 (HV Cet) was extensively followed by Swift to study the evolution of its X-ray and UV emission.

Citation Formats

M. O. Arabaci et al., “Detection of a large Be circumstellar disk during X-ray quiescence of XTE J1946+274,” ASTRONOMY & ASTROPHYSICS, pp. 0–0, 2015, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/68513.