Rotationally modulated variations and the mean longitudinal magnetic field of the Herbig Ae star HD 101412
Context. Despite the importance of magnetic fields to a full understanding of the properties of accreting Herbig Ae/Be stars, these fields have scarcely been studied until now over the rotation cycle. One reason for the paucity of these observations is the lack of knowledge of their rotation periods...
Gespeichert in:
Veröffentlicht in: | Astronomy and astrophysics (Berlin) 2011-01, Vol.525, p.L4 |
---|---|
Hauptverfasser: | , , , , , , , , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | |
---|---|
container_issue | |
container_start_page | L4 |
container_title | Astronomy and astrophysics (Berlin) |
container_volume | 525 |
creator | Hubrig, S. Mikulášek, Z. González, J. F. Schöller, M. Ilyin, I. Curé, M. Zejda, M. Cowley, C. R. Elkin, V. G. Pogodin, M. A. Yudin, R. V. |
description | Context. Despite the importance of magnetic fields to a full understanding of the properties of accreting Herbig Ae/Be stars, these fields have scarcely been studied until now over the rotation cycle. One reason for the paucity of these observations is the lack of knowledge of their rotation periods. The sharp-lined young Herbig Ae star HD 101412 with a strong surface magnetic field has become in the past few years one of the most well-studied targets among the Herbig Ae/Be stars. Aims. We present our multi-epoch polarimetric spectra of this star acquired with FORS 2 to search for a rotation period and constrain the geometry of the magnetic field. Methods. We measured longitudinal magnetic fields for 13 different epochs distributed over 62 days. These new measurements and our previous measurements of the magnetic field in this star were combined with available photometric observations to determine the rotation period. Results. We find the rotation period to be P = 42.076 ± 0.017 d. According to near-infrared imaging studies, the star is observed nearly edge-on. The star exhibits a single-wave variation in the longitudinal magnetic field during the stellar rotation cycle. These observations are usually considered as evidence of a dominant dipolar contribution to the magnetic field topology. |
doi_str_mv | 10.1051/0004-6361/201015806 |
format | Article |
fullrecord | <record><control><sourceid>istex_cross</sourceid><recordid>TN_cdi_crossref_primary_10_1051_0004_6361_201015806</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>ark_67375_80W_4ZC7S78F_T</sourcerecordid><originalsourceid>FETCH-LOGICAL-c468t-a7e952a5e31246a0b51397b4df332a1300a9444e8ff3d96853552f3cf98974e13</originalsourceid><addsrcrecordid>eNo9kN1KAzEQRoMoWKtP4E1eYG3-k70s1VqhIGhF8CZMd5Oaut2VJBX79m5b6dXwDd8ZhoPQLSV3lEg6IoSIQnFFR4xQQqUh6gwNqOCsIFqoczQ4NS7RVUrrPjJq-ACtX7oMOXQtNM0Ob7p620B2Nf6BGA77hKGtcf50eOOgxU3XrkLe1qEH8AZWrcuhwj64psadP_RmLi7DCo8dThkint3j_iVB2TW68NAkd_M_h-ht-rCYzIr58-PTZDwvKqFMLkC7UjKQjlMmFJClpLzUS1F7zhlQTgiUQghnvOd1qYzkUjLPK1-aUgtH-RDx490qdilF5-13DBuIO0uJ3euyexl2L8OedPVUcaRCyu73hED8skpzLa0h71Z8TPSrNlO74H94KWrO</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Rotationally modulated variations and the mean longitudinal magnetic field of the Herbig Ae star HD 101412</title><source>Bacon EDP Sciences France Licence nationale-ISTEX-PS-Journals-PFISTEX</source><source>Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals</source><source>EDP Sciences</source><creator>Hubrig, S. ; Mikulášek, Z. ; González, J. F. ; Schöller, M. ; Ilyin, I. ; Curé, M. ; Zejda, M. ; Cowley, C. R. ; Elkin, V. G. ; Pogodin, M. A. ; Yudin, R. V.</creator><creatorcontrib>Hubrig, S. ; Mikulášek, Z. ; González, J. F. ; Schöller, M. ; Ilyin, I. ; Curé, M. ; Zejda, M. ; Cowley, C. R. ; Elkin, V. G. ; Pogodin, M. A. ; Yudin, R. V.</creatorcontrib><description>Context. Despite the importance of magnetic fields to a full understanding of the properties of accreting Herbig Ae/Be stars, these fields have scarcely been studied until now over the rotation cycle. One reason for the paucity of these observations is the lack of knowledge of their rotation periods. The sharp-lined young Herbig Ae star HD 101412 with a strong surface magnetic field has become in the past few years one of the most well-studied targets among the Herbig Ae/Be stars. Aims. We present our multi-epoch polarimetric spectra of this star acquired with FORS 2 to search for a rotation period and constrain the geometry of the magnetic field. Methods. We measured longitudinal magnetic fields for 13 different epochs distributed over 62 days. These new measurements and our previous measurements of the magnetic field in this star were combined with available photometric observations to determine the rotation period. Results. We find the rotation period to be P = 42.076 ± 0.017 d. According to near-infrared imaging studies, the star is observed nearly edge-on. The star exhibits a single-wave variation in the longitudinal magnetic field during the stellar rotation cycle. These observations are usually considered as evidence of a dominant dipolar contribution to the magnetic field topology.</description><identifier>ISSN: 0004-6361</identifier><identifier>EISSN: 1432-0746</identifier><identifier>DOI: 10.1051/0004-6361/201015806</identifier><language>eng</language><publisher>EDP Sciences</publisher><subject>stars: atmospheres ; stars: individual: HD 101412 ; stars: magnetic field ; stars: pre-main sequence ; stars: rotation ; stars: variables: general</subject><ispartof>Astronomy and astrophysics (Berlin), 2011-01, Vol.525, p.L4</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c468t-a7e952a5e31246a0b51397b4df332a1300a9444e8ff3d96853552f3cf98974e13</citedby><cites>FETCH-LOGICAL-c468t-a7e952a5e31246a0b51397b4df332a1300a9444e8ff3d96853552f3cf98974e13</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,3727,27924,27925</link.rule.ids></links><search><creatorcontrib>Hubrig, S.</creatorcontrib><creatorcontrib>Mikulášek, Z.</creatorcontrib><creatorcontrib>González, J. F.</creatorcontrib><creatorcontrib>Schöller, M.</creatorcontrib><creatorcontrib>Ilyin, I.</creatorcontrib><creatorcontrib>Curé, M.</creatorcontrib><creatorcontrib>Zejda, M.</creatorcontrib><creatorcontrib>Cowley, C. R.</creatorcontrib><creatorcontrib>Elkin, V. G.</creatorcontrib><creatorcontrib>Pogodin, M. A.</creatorcontrib><creatorcontrib>Yudin, R. V.</creatorcontrib><title>Rotationally modulated variations and the mean longitudinal magnetic field of the Herbig Ae star HD 101412</title><title>Astronomy and astrophysics (Berlin)</title><description>Context. Despite the importance of magnetic fields to a full understanding of the properties of accreting Herbig Ae/Be stars, these fields have scarcely been studied until now over the rotation cycle. One reason for the paucity of these observations is the lack of knowledge of their rotation periods. The sharp-lined young Herbig Ae star HD 101412 with a strong surface magnetic field has become in the past few years one of the most well-studied targets among the Herbig Ae/Be stars. Aims. We present our multi-epoch polarimetric spectra of this star acquired with FORS 2 to search for a rotation period and constrain the geometry of the magnetic field. Methods. We measured longitudinal magnetic fields for 13 different epochs distributed over 62 days. These new measurements and our previous measurements of the magnetic field in this star were combined with available photometric observations to determine the rotation period. Results. We find the rotation period to be P = 42.076 ± 0.017 d. According to near-infrared imaging studies, the star is observed nearly edge-on. The star exhibits a single-wave variation in the longitudinal magnetic field during the stellar rotation cycle. These observations are usually considered as evidence of a dominant dipolar contribution to the magnetic field topology.</description><subject>stars: atmospheres</subject><subject>stars: individual: HD 101412</subject><subject>stars: magnetic field</subject><subject>stars: pre-main sequence</subject><subject>stars: rotation</subject><subject>stars: variables: general</subject><issn>0004-6361</issn><issn>1432-0746</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2011</creationdate><recordtype>article</recordtype><recordid>eNo9kN1KAzEQRoMoWKtP4E1eYG3-k70s1VqhIGhF8CZMd5Oaut2VJBX79m5b6dXwDd8ZhoPQLSV3lEg6IoSIQnFFR4xQQqUh6gwNqOCsIFqoczQ4NS7RVUrrPjJq-ACtX7oMOXQtNM0Ob7p620B2Nf6BGA77hKGtcf50eOOgxU3XrkLe1qEH8AZWrcuhwj64psadP_RmLi7DCo8dThkint3j_iVB2TW68NAkd_M_h-ht-rCYzIr58-PTZDwvKqFMLkC7UjKQjlMmFJClpLzUS1F7zhlQTgiUQghnvOd1qYzkUjLPK1-aUgtH-RDx490qdilF5-13DBuIO0uJ3euyexl2L8OedPVUcaRCyu73hED8skpzLa0h71Z8TPSrNlO74H94KWrO</recordid><startdate>20110101</startdate><enddate>20110101</enddate><creator>Hubrig, S.</creator><creator>Mikulášek, Z.</creator><creator>González, J. F.</creator><creator>Schöller, M.</creator><creator>Ilyin, I.</creator><creator>Curé, M.</creator><creator>Zejda, M.</creator><creator>Cowley, C. R.</creator><creator>Elkin, V. G.</creator><creator>Pogodin, M. A.</creator><creator>Yudin, R. V.</creator><general>EDP Sciences</general><scope>BSCLL</scope><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>20110101</creationdate><title>Rotationally modulated variations and the mean longitudinal magnetic field of the Herbig Ae star HD 101412</title><author>Hubrig, S. ; Mikulášek, Z. ; González, J. F. ; Schöller, M. ; Ilyin, I. ; Curé, M. ; Zejda, M. ; Cowley, C. R. ; Elkin, V. G. ; Pogodin, M. A. ; Yudin, R. V.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c468t-a7e952a5e31246a0b51397b4df332a1300a9444e8ff3d96853552f3cf98974e13</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2011</creationdate><topic>stars: atmospheres</topic><topic>stars: individual: HD 101412</topic><topic>stars: magnetic field</topic><topic>stars: pre-main sequence</topic><topic>stars: rotation</topic><topic>stars: variables: general</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Hubrig, S.</creatorcontrib><creatorcontrib>Mikulášek, Z.</creatorcontrib><creatorcontrib>González, J. F.</creatorcontrib><creatorcontrib>Schöller, M.</creatorcontrib><creatorcontrib>Ilyin, I.</creatorcontrib><creatorcontrib>Curé, M.</creatorcontrib><creatorcontrib>Zejda, M.</creatorcontrib><creatorcontrib>Cowley, C. R.</creatorcontrib><creatorcontrib>Elkin, V. G.</creatorcontrib><creatorcontrib>Pogodin, M. A.</creatorcontrib><creatorcontrib>Yudin, R. V.</creatorcontrib><collection>Istex</collection><collection>CrossRef</collection><jtitle>Astronomy and astrophysics (Berlin)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Hubrig, S.</au><au>Mikulášek, Z.</au><au>González, J. F.</au><au>Schöller, M.</au><au>Ilyin, I.</au><au>Curé, M.</au><au>Zejda, M.</au><au>Cowley, C. R.</au><au>Elkin, V. G.</au><au>Pogodin, M. A.</au><au>Yudin, R. V.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Rotationally modulated variations and the mean longitudinal magnetic field of the Herbig Ae star HD 101412</atitle><jtitle>Astronomy and astrophysics (Berlin)</jtitle><date>2011-01-01</date><risdate>2011</risdate><volume>525</volume><spage>L4</spage><pages>L4-</pages><issn>0004-6361</issn><eissn>1432-0746</eissn><abstract>Context. Despite the importance of magnetic fields to a full understanding of the properties of accreting Herbig Ae/Be stars, these fields have scarcely been studied until now over the rotation cycle. One reason for the paucity of these observations is the lack of knowledge of their rotation periods. The sharp-lined young Herbig Ae star HD 101412 with a strong surface magnetic field has become in the past few years one of the most well-studied targets among the Herbig Ae/Be stars. Aims. We present our multi-epoch polarimetric spectra of this star acquired with FORS 2 to search for a rotation period and constrain the geometry of the magnetic field. Methods. We measured longitudinal magnetic fields for 13 different epochs distributed over 62 days. These new measurements and our previous measurements of the magnetic field in this star were combined with available photometric observations to determine the rotation period. Results. We find the rotation period to be P = 42.076 ± 0.017 d. According to near-infrared imaging studies, the star is observed nearly edge-on. The star exhibits a single-wave variation in the longitudinal magnetic field during the stellar rotation cycle. These observations are usually considered as evidence of a dominant dipolar contribution to the magnetic field topology.</abstract><pub>EDP Sciences</pub><doi>10.1051/0004-6361/201015806</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0004-6361 |
ispartof | Astronomy and astrophysics (Berlin), 2011-01, Vol.525, p.L4 |
issn | 0004-6361 1432-0746 |
language | eng |
recordid | cdi_crossref_primary_10_1051_0004_6361_201015806 |
source | Bacon EDP Sciences France Licence nationale-ISTEX-PS-Journals-PFISTEX; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; EDP Sciences |
subjects | stars: atmospheres stars: individual: HD 101412 stars: magnetic field stars: pre-main sequence stars: rotation stars: variables: general |
title | Rotationally modulated variations and the mean longitudinal magnetic field of the Herbig Ae star HD 101412 |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-22T18%3A18%3A10IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-istex_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Rotationally%20modulated%20variations%20and%20the%20mean%20longitudinal%20magnetic%20field%20of%20the%20Herbig%20Ae%20star%20HD%20101412&rft.jtitle=Astronomy%20and%20astrophysics%20(Berlin)&rft.au=Hubrig,%20S.&rft.date=2011-01-01&rft.volume=525&rft.spage=L4&rft.pages=L4-&rft.issn=0004-6361&rft.eissn=1432-0746&rft_id=info:doi/10.1051/0004-6361/201015806&rft_dat=%3Cistex_cross%3Eark_67375_80W_4ZC7S78F_T%3C/istex_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true |