Quiescent and Active States of V1413 Aql I: Photometric Activity Criterion and the Detection of a Secondary Minimum
We present the results of our photometric UBV JHKL observations for the symbiotic star V1413 Aql obtained in 2012–2018. An analysis of the data has shown that inMay 2017 the system passed to a quiescent state with B − V ≈ 0 ṃ 6 for the first time since 1993. It lasted no more than five months. The J...
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| Veröffentlicht in: | Astronomy letters 2018-12, Vol.44 (12), p.803-810 |
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| container_title | Astronomy letters |
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| creator | Tatarnikova, A. A. Tatarnikov, A. M. Kolotilov, E. A. Shenavrin, V. I. Komissarova, G. V. |
| description | We present the results of our photometric
UBV JHKL
observations for the symbiotic star V1413 Aql obtained in 2012–2018. An analysis of the data has shown that inMay 2017 the system passed to a quiescent state with
B − V
≈ 0
ṃ
6 for the first time since 1993. It lasted no more than five months. The
J − K
color at the primary minimum of 2012 reached 1
ṃ
5, which, given the interstellar reddening, corresponds to spectral type M5-M6 III of the cool component. A secondary minimum has been detected at
φ
≈ 0.5 on the JK phase light curves constructed for the dates of observations with
B
≥ 13. |
| doi_str_mv | 10.1134/S106377371812006X |
| format | Article |
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UBV JHKL
observations for the symbiotic star V1413 Aql obtained in 2012–2018. An analysis of the data has shown that inMay 2017 the system passed to a quiescent state with
B − V
≈ 0
ṃ
6 for the first time since 1993. It lasted no more than five months. The
J − K
color at the primary minimum of 2012 reached 1
ṃ
5, which, given the interstellar reddening, corresponds to spectral type M5-M6 III of the cool component. A secondary minimum has been detected at
φ
≈ 0.5 on the JK phase light curves constructed for the dates of observations with
B
≥ 13.</description><identifier>ISSN: 1063-7737</identifier><identifier>EISSN: 1562-6873</identifier><identifier>DOI: 10.1134/S106377371812006X</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>Astronomy ; Astrophysics and Astroparticles ; Interstellar extinction ; Monte Carlo simulation ; Observations and Techniques ; Photometry ; Physics ; Physics and Astronomy ; Symbiotic stars</subject><ispartof>Astronomy letters, 2018-12, Vol.44 (12), p.803-810</ispartof><rights>Pleiades Publishing, Inc. 2018</rights><rights>Astronomy Letters is a copyright of Springer, (2018). All Rights Reserved.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c316t-1d0cc8e6a0b5ff9e63ed68578e907b665bc380b99d7d743324a9ead901d2d88c3</citedby><cites>FETCH-LOGICAL-c316t-1d0cc8e6a0b5ff9e63ed68578e907b665bc380b99d7d743324a9ead901d2d88c3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1134/S106377371812006X$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1134/S106377371812006X$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,776,780,27901,27902,41464,42533,51294</link.rule.ids></links><search><creatorcontrib>Tatarnikova, A. A.</creatorcontrib><creatorcontrib>Tatarnikov, A. M.</creatorcontrib><creatorcontrib>Kolotilov, E. A.</creatorcontrib><creatorcontrib>Shenavrin, V. I.</creatorcontrib><creatorcontrib>Komissarova, G. V.</creatorcontrib><title>Quiescent and Active States of V1413 Aql I: Photometric Activity Criterion and the Detection of a Secondary Minimum</title><title>Astronomy letters</title><addtitle>Astron. Lett</addtitle><description>We present the results of our photometric
UBV JHKL
observations for the symbiotic star V1413 Aql obtained in 2012–2018. An analysis of the data has shown that inMay 2017 the system passed to a quiescent state with
B − V
≈ 0
ṃ
6 for the first time since 1993. It lasted no more than five months. The
J − K
color at the primary minimum of 2012 reached 1
ṃ
5, which, given the interstellar reddening, corresponds to spectral type M5-M6 III of the cool component. A secondary minimum has been detected at
φ
≈ 0.5 on the JK phase light curves constructed for the dates of observations with
B
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V.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c316t-1d0cc8e6a0b5ff9e63ed68578e907b665bc380b99d7d743324a9ead901d2d88c3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2018</creationdate><topic>Astronomy</topic><topic>Astrophysics and Astroparticles</topic><topic>Interstellar extinction</topic><topic>Monte Carlo simulation</topic><topic>Observations and Techniques</topic><topic>Photometry</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Symbiotic stars</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Tatarnikova, A. A.</creatorcontrib><creatorcontrib>Tatarnikov, A. M.</creatorcontrib><creatorcontrib>Kolotilov, E. A.</creatorcontrib><creatorcontrib>Shenavrin, V. I.</creatorcontrib><creatorcontrib>Komissarova, G. 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UBV JHKL
observations for the symbiotic star V1413 Aql obtained in 2012–2018. An analysis of the data has shown that inMay 2017 the system passed to a quiescent state with
B − V
≈ 0
ṃ
6 for the first time since 1993. It lasted no more than five months. The
J − K
color at the primary minimum of 2012 reached 1
ṃ
5, which, given the interstellar reddening, corresponds to spectral type M5-M6 III of the cool component. A secondary minimum has been detected at
φ
≈ 0.5 on the JK phase light curves constructed for the dates of observations with
B
≥ 13.</abstract><cop>Moscow</cop><pub>Pleiades Publishing</pub><doi>10.1134/S106377371812006X</doi><tpages>8</tpages></addata></record> |
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| subjects | Astronomy Astrophysics and Astroparticles Interstellar extinction Monte Carlo simulation Observations and Techniques Photometry Physics Physics and Astronomy Symbiotic stars |
| title | Quiescent and Active States of V1413 Aql I: Photometric Activity Criterion and the Detection of a Secondary Minimum |
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