Hard X-ray Emission of Intermediate polars

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F10%3A00373414" target="_blank" >RIV/67985815:_____/10:00373414 - isvavai.cz</a>

Result on the web

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DOI - Digital Object Identifier

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Result language

angličtina

Original language name

Hard X-ray Emission of Intermediate polars

Original language description

Our analysis based on observational data from INTEGRAL/IBIS and INTEGRAL/JEM-X showed that the f uxes of some intermediate polars are long-term variable. Moreover, this hard X-ray/soft ?- ray variability is correlated with the changes in optical spectralband. The broad-band spectra (3 - 100 keV) of surveyed intermediate polars can be well f tted by a thermal bremsstrahlung model with ref ection from the surface of the white dwarf in some cases.

Czech name

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Czech description

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Type

D - Article in proceedings

CEP classification

BN - Astronomy and celestial mechanics, astrophysics

OECD FORD branch

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Project

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Continuities

Z - Vyzkumny zamer (s odkazem do CEZ)

Publication year

2010

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection

Binaries - Key to Comprehension of the Universe

ISBN

978-1-58381-750-6

ISSN

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e-ISSN

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Number of pages

4

Pages from-to

311-314

Publisher name

Astronomical Society of the Pacific

Place of publication

San Francisco

Event location

Brno

Event date

Jun 8, 2009

Type of event by nationality

WRD - Celosvětová akce

UT code for WoS article

000289880000072