CCD photometry of outbursts in GK Per.
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F01%3A01010102" target="_blank" >RIV/67985815:_____/01:01010102 - isvavai.cz</a>
Result on the web
—
DOI - Digital Object Identifier
—
Alternative languages
Result language
angličtina
Original language name
CCD photometry of outbursts in GK Per.
Original language description
Photometry of the dwarf nova type 1996 outburst of GK Per shows that the color indices are getting bluer during the late rise to the maximum brightness and a strong linear reddening is visible during the decline. The brightness fluctuations were detectedduring the 1999 outburst. The amplitude of the fluctuations was increasing during the rise to the maximum light.
Czech name
—
Czech description
—
Classification
Type
D - Article in proceedings
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
—
Result continuities
Project
<a href="/en/project/ME%20137" target="_blank" >ME 137: XMM-The X-ray Multi-Mirror Satellite</a><br>
Continuities
Z - Vyzkumny zamer (s odkazem do CEZ)
Others
Publication year
2001
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
X-ray astronomy. Stellar endpoints, AGN, and the diffuse background.
ISBN
—
ISSN
—
e-ISSN
—
Number of pages
4
Pages from-to
939-942
Publisher name
American Institute of Physics
Place of publication
Melville
Event location
Bologna [IT]
Event date
Sep 6, 1999
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
—