Observations of Candidates for Eclipsing Cataclysmic Variables with the RTT-150 Telescope
We present the results of our photometric and spectroscopic observations. We have studied four cataclysmic variable stars: 2XMM J183251.4-100106, MLS1809017 J224712+461815, MGAB-V330, and MGAB-V410. We have analyzed the observational data and determined the periods of the systems from our photometri...
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| Veröffentlicht in: | Astronomy letters 2021-10, Vol.47 (10), p.695-704 |
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| creator | Gabdeev, M. M. Bikmaev, I. F. Shimansky, V. V. Zhuchkov, R. Ya Irtuganov, E. N. |
| description | We present the results of our photometric and spectroscopic observations. We have studied four cataclysmic variable stars: 2XMM J183251.4-100106, MLS1809017 J224712+461815, MGAB-V330, and MGAB-V410. We have analyzed the observational data and determined the periods of the systems from our photometric data. The object MLS1809017 J224712+461815 has been classified as an SU UMa-type dwarf nova. The remaining three systems are eclipsing ones, with 2XMM J183251.4-100106 and MGAB-V410 showing signatures of polars. At the same time, for MGAB-V410 the orbital period
falls into the period gap for cataclysmic variables. |
| doi_str_mv | 10.1134/S1063773721100042 |
| format | Article |
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falls into the period gap for cataclysmic variables.</description><subject>Astronomy</subject><subject>Astrophysics and Astroparticles</subject><subject>Cataclysmic variables</subject><subject>Dwarf novae</subject><subject>Observations and Techniques</subject><subject>Orbits</subject><subject>Photometry</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Spectroscopic observation</subject><subject>Variable stars</subject><issn>1063-7737</issn><issn>1562-6873</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><recordid>eNp1kFFLwzAQx4MoOKcfwLeAz9W7pG26RxnTCYOBVsGnkqbpltE1NcmUfXszJvgg3ssd9__977gj5BrhFpGndy8IOReCC4YIACk7ISPMcpbkheCnsY5yctDPyYX3m4hMOIcReV_WXrtPGYztPbUtncq-MY0M2tPWOjpTnRm86VdRCFJ1e781ir5JZ2TdRebLhDUNa02fyzLBDGipY1vZQV-Ss1Z2Xl_95DF5fZiV03myWD4-Te8XiWJ5EZIJCtYInqZKAs9YLhkUBTBoWVOoFpXAWvKaMZ1qDTXHiWgAIVOZlEIV8bgxuTnOHZz92Gkfqo3duT6urFjOgRVZjEjhkVLOeu90Ww3ObKXbVwjV4YPVnw9GDzt6fGT7lXa_k_83fQPfgHCY</recordid><startdate>20211001</startdate><enddate>20211001</enddate><creator>Gabdeev, M. M.</creator><creator>Bikmaev, I. F.</creator><creator>Shimansky, V. V.</creator><creator>Zhuchkov, R. Ya</creator><creator>Irtuganov, E. N.</creator><general>Pleiades Publishing</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope></search><sort><creationdate>20211001</creationdate><title>Observations of Candidates for Eclipsing Cataclysmic Variables with the RTT-150 Telescope</title><author>Gabdeev, M. M. ; Bikmaev, I. F. ; Shimansky, V. V. ; Zhuchkov, R. Ya ; Irtuganov, E. N.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c268t-9172d7344ca03526a2088020f2d8cf1c71ba3b22e4ee0b3197d0105c5aa7c8873</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>Astronomy</topic><topic>Astrophysics and Astroparticles</topic><topic>Cataclysmic variables</topic><topic>Dwarf novae</topic><topic>Observations and Techniques</topic><topic>Orbits</topic><topic>Photometry</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Spectroscopic observation</topic><topic>Variable stars</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Gabdeev, M. M.</creatorcontrib><creatorcontrib>Bikmaev, I. F.</creatorcontrib><creatorcontrib>Shimansky, V. V.</creatorcontrib><creatorcontrib>Zhuchkov, R. Ya</creatorcontrib><creatorcontrib>Irtuganov, E. N.</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Astronomy letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Gabdeev, M. M.</au><au>Bikmaev, I. F.</au><au>Shimansky, V. V.</au><au>Zhuchkov, R. Ya</au><au>Irtuganov, E. N.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Observations of Candidates for Eclipsing Cataclysmic Variables with the RTT-150 Telescope</atitle><jtitle>Astronomy letters</jtitle><stitle>Astron. Lett</stitle><date>2021-10-01</date><risdate>2021</risdate><volume>47</volume><issue>10</issue><spage>695</spage><epage>704</epage><pages>695-704</pages><issn>1063-7737</issn><eissn>1562-6873</eissn><abstract>We present the results of our photometric and spectroscopic observations. We have studied four cataclysmic variable stars: 2XMM J183251.4-100106, MLS1809017 J224712+461815, MGAB-V330, and MGAB-V410. We have analyzed the observational data and determined the periods of the systems from our photometric data. The object MLS1809017 J224712+461815 has been classified as an SU UMa-type dwarf nova. The remaining three systems are eclipsing ones, with 2XMM J183251.4-100106 and MGAB-V410 showing signatures of polars. At the same time, for MGAB-V410 the orbital period
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| subjects | Astronomy Astrophysics and Astroparticles Cataclysmic variables Dwarf novae Observations and Techniques Orbits Photometry Physics Physics and Astronomy Spectroscopic observation Variable stars |
| title | Observations of Candidates for Eclipsing Cataclysmic Variables with the RTT-150 Telescope |
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