dc.contributor.author |
Vinokurov, A |
|
dc.contributor.author |
Atapin, K |
|
dc.contributor.author |
Bordoloi, O. P |
|
dc.contributor.author |
Sarkisyan, A |
|
dc.contributor.author |
Kashyap, U |
|
dc.contributor.author |
Chakraborty, M |
|
dc.contributor.author |
Rahna, P. T |
|
dc.contributor.author |
Kostenkov, A |
|
dc.contributor.author |
Solovyeva, Y |
|
dc.contributor.author |
Fabrika, S |
|
dc.contributor.author |
Safonova, M |
|
dc.contributor.author |
Gogoi, R |
|
dc.contributor.author |
Sutaria, F. K |
|
dc.contributor.author |
Murthy, J |
|
dc.date.accessioned |
2022-10-21T09:01:00Z |
|
dc.date.available |
2022-10-21T09:01:00Z |
|
dc.date.issued |
2022-09 |
|
dc.identifier.citation |
Astrophysical Bulletin, Vol. 77, No. 3, pp. 231–245 |
en_US |
dc.identifier.issn |
1990-3421 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/8068 |
|
dc.description |
Restricted Access |
en_US |
dc.description |
The original publication is available at the springerlink.com |
|
dc.description.abstract |
We present the results of eight epochs of simultaneous UV and X-ray observations of the highly variable ultraluminous X-ray source (ULX) Holmberg II X-1 with AstroSat—Indian multiwavelength space satellite. During the entire observation period from late 2016 to early 2020, Holmberg II X-1 showed a moderate X-ray luminosity about of 8×10398×1039 erg s−1−1 and a hard power-law spectrum with Γ≲1.9Γ≲1.9. Due to low variability of the object in X-rays (by a factor 1.5) and insignificant variability in the UV range (upper limit approximately 25%) we could not find reliable correlation between flux changes in these ranges. Inside each particular observation, the X-ray variability amplitude is higher, reaching a factor of 2–3 respect to the mean level, however, it is observed in the form of relatively short stochastic bursts. We discussed our results in terms of three models of a heated donor star, a heated disk and a heated wind, and estimated the lower limit to the variability which would allow to reject at least part of them. |
en_US |
dc.language.iso |
en |
en_US |
dc.publisher |
Springer |
en_US |
dc.relation.uri |
https://doi.org/10.1134/S1990341322030129 |
|
dc.rights |
©The Author(s) |
|
dc.subject |
Accretion |
en_US |
dc.subject |
Accretion disks |
en_US |
dc.subject |
X-rays: binaries |
en_US |
dc.subject |
X-rays: individual: Holmberg II X-1 |
en_US |
dc.title |
Simultaneous X-ray/UV Observations of Ultraluminous X-ray Source Holmberg II X-1 with Indian Space Mission Astrosat |
en_US |
dc.type |
Article |
en_US |