Studying the Magnetic Properties of Upper Main-sequence Stars with FORS1

[en] We summarise the results of our recent magnetic field studies in upper main-sequence stars, which have exploited the spectropolarimetric capability of FORS1 at the VLT extensively.

Disciplines :

Space science, astronomy & astrophysics

Author, co-author :

Hubrig, Swetlana; ESO ; Astrophysikalisches Institut Potsdam, Germany) AB(ESO) AC(Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Belgium) AD(Koninklijke Sterrenwacht van BelgiÃ«, Brussel, Belgium) AE(Institut d'Astrophysique et de GÃ©ophysique, UniversitÃ© de LiÃ¨ge, Belgium) AF(Centre for Astrophysics, University of Central Lancashire, Preston, UK) AG(Centre for Astrophysics, University of Central Lancashire, Preston, UK) AH(INAF-Osservatorio Astronomico di Palermo, Italy) AI(Institute for Solar Physics, Royal Swedish Academy of Sciences, Stockholm, Sweden) AJ(Eureka Scientific, Oakland, USA) AK(Pulkovo Observatory, Saint- Petersburg, Russia ; Isaac Newton Institute of Chile, Saint-Petersburg Branch, Russia) AL(ESO) AM(Departamento de FÃsica y AstronomÃa, Universidad de ValparaÃso, Chile) AN(Pulkovo Observatory, Saint- Petersburg, Russia ; Isaac Newton Institute of Chile, Saint-Petersburg Branch, Russia) AO(ESO

Scholler, Markus

Briquet, Maryline

De Cat, Peter

Morel, Thierry ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Groupe d'astrophysique des hautes énergies (GAPHE)

Kurtz, Donald

Elkin, Vladimir

Stelzer, Beate

Schnerr, Roald

Grady, Carol

More authors (5 more)

Language :

English

Title :

Studying the Magnetic Properties of Upper Main-sequence Stars with FORS1

Publication date :

01 March 2009

Journal title :

Messenger

ISSN :

0722-6691

Publisher :

European Southern Observatory, Garching, Germany

Volume :

135

Pages :

21-25

Additional URL :

http://adsabs.harvard.edu/abs/2009Msngr.135...21H

Available on ORBi :

since 19 February 2010

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