The outburst of Nova CSS 081007:030559+054715 (HV Ceti)

Download

Date

2012-09-01

Author

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.

Metadata

Show full item record

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

Item Usage Stats

141
views

0
downloads

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.

Subject Keywords

Novae, cataclysmic variables, Stars: individual: CSS 081007: 030559+054715 (HV Cet), X-rays: stars, Ultraviolet: stars

URI

https://hdl.handle.net/11511/49791

Journal

ASTRONOMY & ASTROPHYSICS

DOI

https://doi.org/10.1051/0004-6361/201219681

Collections

Department of Physics, Article

Suggestions

OpenMETU
Core

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.
Detection of a large Be circumstellar disk during X-ray quiescence of XTE J1946+274 Arabaci, M. Ozbey; Camero-Arranz, A.; Zurita, C.; Gutierrez-Soto, J.; Nespoli, E.; Suso, J.; Kiaeerad, F.; Garcia-Rojas, J.; Kiziloglu, U. (2015-10-01) 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.
Activity from the Be/X-ray binary system V0332+53 during its intermediate-luminosity outburst in 2008 Caballero-Garcia, M. D.; Camero-Arranz, A.; Arabaci, M. Ozbey; Zurita, C.; Suso, J.; Gutierrez-Soto, J.; BEKLEN BARTO, Elif; Kiaeerad, F.; Garrido, R.; Hudec, R. (EDP Sciences, 2016-05-01) Aims. We present a study of the Be/X-ray binary system V 0332+53 with the main goal of characterizing its behaviour mainly during the intermediate-luminosity X-ray event in 2008. In addition, we aim to contribute to the understanding of the behaviour of the donor companion by including optical data from our dedicated campaign starting in 2006.
Recent RXTE/ASM and ROTSEIIId observations of EXO 2030+375 (V2246 Cygni) Baykal, Altan; Kiziloglu, N.; Beklen, E.; Oezbey, M. (EDP Sciences, 2008-02-01) Aims. Using the archival RXTE/ASM and SWIFT/BAT observations, the new orbital phases of type I outbursts of EXO 2030+375 are estimated. A possible correlation between the type II outburst and optical brightness variations is investigated.

Citation Formats

A. P. Beardmore et al., “The outburst of Nova CSS 081007:030559+054715 (HV Ceti),” ASTRONOMY & ASTROPHYSICS, pp. 0–0, 2012, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/49791.