Photometric monitoring of the young star Par 1724 in Orion
We report new photometric observations of the ∼200 000 year old naked weak‐line run‐away T Tauri star Par 1724, located north of the Trapezium cluster in Orion. We observed in the broad band filters B, V, R, and I using the 90 cm Dutch telescope on La Silla, the 80 cm Wendelstein telescope, and a 25...
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| Veröffentlicht in: | Astronomische Nachrichten 2009-06, Vol.330 (5), p.493-503 |
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| creator | Neuhäuser, R. Koeltzsch, A. Raetz, St Schmidt, T. O. B. Mugrauer, M. Young, N. Bertoldi, F. Roell, T. Eisenbeiss, T. Hohle, M. M. Vaňko, M. Ginski, C. Rammo, W. Moualla, M. Broeg, C. |
| description | We report new photometric observations of the ∼200 000 year old naked weak‐line run‐away T Tauri star Par 1724, located north of the Trapezium cluster in Orion. We observed in the broad band filters B, V, R, and I using the 90 cm Dutch telescope on La Silla, the 80 cm Wendelstein telescope, and a 25 cm telescope of the University Observatory Jena in Großschwabhausen near Jena. The photometric data in V and R are consistent with a ∼5.7 day rotation period due to spots, as observed before between 1960ies and 2000. Also, for the first time, we present evidence for a long‐term 9 or 17.5 year cycle in photometric data (V band) of such a young star, a cycle similar to that to of the Sun and other active stars (© 2009 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim) |
| doi_str_mv | 10.1002/asna.200911196 |
| format | Article |
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O. B. ; Mugrauer, M. ; Young, N. ; Bertoldi, F. ; Roell, T. ; Eisenbeiss, T. ; Hohle, M. M. ; Vaňko, M. ; Ginski, C. ; Rammo, W. ; Moualla, M. ; Broeg, C.</creator><creatorcontrib>Neuhäuser, R. ; Koeltzsch, A. ; Raetz, St ; Schmidt, T. O. B. ; Mugrauer, M. ; Young, N. ; Bertoldi, F. ; Roell, T. ; Eisenbeiss, T. ; Hohle, M. M. ; Vaňko, M. ; Ginski, C. ; Rammo, W. ; Moualla, M. ; Broeg, C.</creatorcontrib><description>We report new photometric observations of the ∼200 000 year old naked weak‐line run‐away T Tauri star Par 1724, located north of the Trapezium cluster in Orion. We observed in the broad band filters B, V, R, and I using the 90 cm Dutch telescope on La Silla, the 80 cm Wendelstein telescope, and a 25 cm telescope of the University Observatory Jena in Großschwabhausen near Jena. The photometric data in V and R are consistent with a ∼5.7 day rotation period due to spots, as observed before between 1960ies and 2000. Also, for the first time, we present evidence for a long‐term 9 or 17.5 year cycle in photometric data (V band) of such a young star, a cycle similar to that to of the Sun and other active stars (© 2009 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)</description><identifier>ISSN: 0004-6337</identifier><identifier>EISSN: 1521-3994</identifier><identifier>DOI: 10.1002/asna.200911196</identifier><language>eng</language><publisher>Berlin: WILEY-VCH Verlag</publisher><subject>stars: individual (Par 1724) ; stars: late-type ; stars: pre-main sequence ; stars: rotation ; T Tauri stars</subject><ispartof>Astronomische Nachrichten, 2009-06, Vol.330 (5), p.493-503</ispartof><rights>Copyright © 2009 WILEY‐VCH Verlag GmbH & Co. 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M.</au><au>Vaňko, M.</au><au>Ginski, C.</au><au>Rammo, W.</au><au>Moualla, M.</au><au>Broeg, C.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Photometric monitoring of the young star Par 1724 in Orion</atitle><jtitle>Astronomische Nachrichten</jtitle><addtitle>Astron. Nachr</addtitle><date>2009-06</date><risdate>2009</risdate><volume>330</volume><issue>5</issue><spage>493</spage><epage>503</epage><pages>493-503</pages><issn>0004-6337</issn><eissn>1521-3994</eissn><abstract>We report new photometric observations of the ∼200 000 year old naked weak‐line run‐away T Tauri star Par 1724, located north of the Trapezium cluster in Orion. We observed in the broad band filters B, V, R, and I using the 90 cm Dutch telescope on La Silla, the 80 cm Wendelstein telescope, and a 25 cm telescope of the University Observatory Jena in Großschwabhausen near Jena. The photometric data in V and R are consistent with a ∼5.7 day rotation period due to spots, as observed before between 1960ies and 2000. Also, for the first time, we present evidence for a long‐term 9 or 17.5 year cycle in photometric data (V band) of such a young star, a cycle similar to that to of the Sun and other active stars (© 2009 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)</abstract><cop>Berlin</cop><pub>WILEY-VCH Verlag</pub><doi>10.1002/asna.200911196</doi><tpages>11</tpages><oa>free_for_read</oa></addata></record> |
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| subjects | stars: individual (Par 1724) stars: late-type stars: pre-main sequence stars: rotation T Tauri stars |
| title | Photometric monitoring of the young star Par 1724 in Orion |
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