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
Reanalysis of high-resolution XMM-Newton data of V2491 Cygni using models of collisionally ionized hot absorbers
Download
index.pdf
Date
2017-02-01
Author
Balman, Şölen
Gamsizkan, C.
Metadata
Show full item record
This work is licensed under a
Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License
.
Item Usage Stats
156
views
0
downloads
Cite This
Aims. We model spectral absorption features in data of the high-resolution XMM-Newton Reflection Grating Spectrometer.
Subject Keywords
X-rays: stars
,
Stars: individual: V2491 Cyg
,
Binaries: general
,
Novae, cataclysmic variables
,
Stars: abundances
,
Stars: winds, outflows
URI
https://hdl.handle.net/11511/57268
Journal
ASTRONOMY & ASTROPHYSICS
DOI
https://doi.org/10.1051/0004-6361/201629360
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).
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.
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.
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.
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.
Citation Formats
IEEE
ACM
APA
CHICAGO
MLA
BibTeX
Ş. Balman and C. Gamsizkan, “Reanalysis of high-resolution XMM-Newton data of V2491 Cygni using models of collisionally ionized hot absorbers,”
ASTRONOMY & ASTROPHYSICS
, pp. 0–0, 2017, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/57268.