Show/Hide Menu
Hide/Show Apps
Logout
Türkçe
Türkçe
Search
Search
Login
Login
OpenMETU
OpenMETU
About
About
Open Science Policy
Open Science Policy
Open Access Guideline
Open Access Guideline
Postgraduate Thesis Guideline
Postgraduate Thesis Guideline
Communities & Collections
Communities & Collections
Help
Help
Frequently Asked Questions
Frequently Asked Questions
Guides
Guides
Thesis submission
Thesis submission
MS without thesis term project submission
MS without thesis term project submission
Publication submission with DOI
Publication submission with DOI
Publication submission
Publication submission
Supporting Information
Supporting Information
General Information
General Information
Copyright, Embargo and License
Copyright, Embargo and License
Contact us
Contact us
Optical and X-ray outbursts of Be/X-ray binary system SAX J2103.5+4545
Download
index.pdf
Date
2009-12-01
Author
Kiziloglu, Ue.
Ozbilgen, S.
Kiziloglu, N.
Baykal, Altan
Metadata
Show full item record
This work is licensed under a
Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License
.
Item Usage Stats
160
views
76
downloads
Cite This
Aims. The main goal of this study is to investigate the relationship between the optical and X-ray behaviours of the Be/X-ray binary system SAX J2103.5+4545.
Subject Keywords
Space and Planetary Science
,
Astronomy and Astrophysics
URI
https://hdl.handle.net/11511/38721
Journal
ASTRONOMY & ASTROPHYSICS
DOI
https://doi.org/10.1051/0004-6361/200912638
Collections
Department of Physics, Article
Suggestions
OpenMETU
Core
Optical variabilities in the Be/X-ray binary system - GRO J2058+42 (CXOU J205847.5+414637)
Kiziloglu, Ue.; Kiziloglu, N.; Baykal, Altan; Yerli, Sinan Kaan; Ozbey, M. (EDP Sciences, 2007-08-01)
Aims. We present an analysis of long-term optical monitoring observations and optical spectroscopic observations of the counterpart to CXOU J205847.5+414637 (high-mass X-ray binary system). We search for variability in the light curve of Be star.
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.
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.
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.
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).
Citation Formats
IEEE
ACM
APA
CHICAGO
MLA
BibTeX
U. Kiziloglu, S. Ozbilgen, N. Kiziloglu, and A. Baykal, “Optical and X-ray outbursts of Be/X-ray binary system SAX J2103.5+4545,”
ASTRONOMY & ASTROPHYSICS
, pp. 895–900, 2009, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/38721.