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Searching for a link between the magnetic nature and other observed properties of Herbig Ae/Be stars

Published online by Cambridge University Press:  01 November 2008

Swetlana Hubrig
Affiliation:
ESO, Santiago, Chile; email: shubrig@eso.org
C. Grady
Affiliation:
Eureka Scientific, Oakland, USA
M. Schöller
Affiliation:
ESO, Garching, Germany
O. Schütz
Affiliation:
ESO, Santiago, Chile; email: shubrig@eso.org
B. Stelzer
Affiliation:
INAF-Osservatorio Astronomico di Palermo, Italy
M. Pogodin
Affiliation:
Pulkovo Observatory, St.-Petersburg, Russia
M. Cure
Affiliation:
Univ. de Valparaiso, Chile
R. Yudin
Affiliation:
Pulkovo Observatory, St.-Petersburg, Russia
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Abstract

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We present the results of a new magnetic field survey of Herbig Ae/Be and A debris disk stars. They are used to determine whether magnetic field properties in these stars are correlated with the mass-accretion rate, disk inclinations, companion(s), Silicates, PAHs, or show a more general correlation with age and X-ray emission as expected for the decay of a remnant dynamo.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2009

References

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Hubrig, S., North, P., & Schöller, M. 2007b, AN 328, 475Google Scholar
Hubrig, S., Pogodin, M. A., Yudin, R. V., et al. 2007a, A&A 463, 1039Google Scholar