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Magnetic, chemical and rotational properties of the Herbig Ae/Be binary system HD 72106
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Astronomy and Space Physics.
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2008 (English)In: Contributions of the Astronomical Observatory Skalnaté Pleso, ISSN 1335-1842, Vol. 38, no 2, 245-250 p.Article in journal (Refereed) Published
Abstract [en]

Recently, strong, globally-ordered magnetic fields have been detected in some Herbig Ae and Be (HAeBe) stars, suggesting a possible evolutionary connection to main sequence magnetic chemically peculiar Ap and Bp stars. We have undertaken a detailed study of the binary system HD 72106, which contains a B9 magnetic primary and a HAeBe secondary, using the ESPaDOnS spectropolarimeter mounted on the CFHT. A careful analysis of the very young primary reveals that it has an approximately dipolar magnetic field geometry, strong chemical peculiarities, and strong surface chemical abundance inhomogeneities. Thus the primary is very similar to an Ap/Bp star despite having completed less then 1.5% of its main sequence life, and possible still being on the pre-main sequence. In contrast, a similar analysis of the secondary reveals solar chemical abundances and no magnetic field.

Place, publisher, year, edition, pages
2008. Vol. 38, no 2, 245-250 p.
Keyword [en]
stars : abundances, stars : magnetic fields, stars : chemically peculiar, stars : pre-main sequence, stars : individual : HD 72106
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:uu:diva-149673ISI: 000256514000023OAI: oai:DiVA.org:uu-149673DiVA: diva2:405825
Note
Conference Information: CP/AP Workshop 2007 Vienna, AUSTRIA, SEP 10-14, 2007Available from: 2011-03-23 Created: 2011-03-22 Last updated: 2011-03-23Bibliographically approved

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