PARIMUCHA, S., P. A. DUBOVSKY, I. KUDZEJ, V. BREUS and Karol PETRÍK. About the dependency of the spin maxima on orbital phase in the intermediate polar MU Cam. Contributions of the Astronomical Observatory Skalnaté pleso. 2020, vol. 50, No 2, p. 618-620. ISSN 1335-1842. Available from: https://dx.doi.org/10.31577/caosp.2020.50.2.618. |
Other formats:
BibTeX
LaTeX
RIS
@article{49458, author = {Parimucha, S. and Dubovsky, P. A. and Kudzej, I. and Breus, V. and Petrík, Karol}, article_number = {2}, doi = {http://dx.doi.org/10.31577/caosp.2020.50.2.618}, keywords = {stars: individual: MU Cam; stars: novae; cataclysmic variables; accretion; accretion discs}, language = {eng}, issn = {1335-1842}, journal = {Contributions of the Astronomical Observatory Skalnaté pleso}, title = {About the dependency of the spin maxima on orbital phase in the intermediate polar MU Cam}, url = {http://www.astro.sk/caosp/Eedition/Abstracts/2020/Vol_50/No_2/pp618-620_abstract.html}, volume = {50}, year = {2020} }
TY - JOUR ID - 49458 AU - Parimucha, S. - Dubovsky, P. A. - Kudzej, I. - Breus, V. - Petrík, Karol PY - 2020 TI - About the dependency of the spin maxima on orbital phase in the intermediate polar MU Cam JF - Contributions of the Astronomical Observatory Skalnaté pleso VL - 50 IS - 2 SP - 618-620 EP - 618-620 SN - 13351842 KW - stars: individual: MU Cam KW - stars: novae KW - cataclysmic variables KW - accretion KW - accretion discs UR - http://www.astro.sk/caosp/Eedition/Abstracts/2020/Vol_50/No_2/pp618-620_abstract.html N2 - Long term monitoring of intermediate polars is performed as part of the Inter-Longitude Astronomy campaign. High-quality and long time series observations allow us to investigate fine effects on complex light curves. In the case of MU Cam we have investigated the periodic modulation of the spin phases with the orbital phase. This dependency was already described by Kim et al. (2005). As an explanation they proposed inhomogeneous accretion flow from the secondary. However, based on our new data, we propose as a simple explanation the influence of orbital sidebands in the periodic signal produced by the intermediate polar. This explanation is supported by the fact that the changes in spin maxima phase are observed mainly when the sideband frequency is dominant in the periodogram. ER -
PARIMUCHA, S., P. A. DUBOVSKY, I. KUDZEJ, V. BREUS and Karol PETRÍK. About the dependency of the spin maxima on orbital phase in the intermediate polar MU Cam. \textit{Contributions of the Astronomical Observatory Skalnaté pleso}. 2020, vol.~50, No~2, p.~618-620. ISSN~1335-1842. Available from: https://dx.doi.org/10.31577/caosp.2020.50.2.618.
|