activity
19982026
most citedA high-resolution spectropolarimetric survey of Herbig Ae/Be stars - I. Observations and measurements

263 citations · 4.4k across the 127 of their papers we have counts for

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Showing 2010Show all

17 papers · 1 filter

astro-ph.SR2010★ 24 cited

A detailed spectroscopic analysis of the open cluster NGC 5460

L. Fossati, C. P. Folsom, S. Bagnulo +5

Within the context of a large project aimed at studying early F-, A- and late B-type stars we present the abundance analysis of the photospheres of 21 members of the open cluster N…

astro-ph.SR2010

Tau Sco: discovery of the clones

V. Petit, D. L. Massa, W. L. F. Marcolino +3

The B0.2 V magnetic star tau Sco stands out from the larger population of massive magnetic OB stars due to its high X-ray activity and remarkable wind, apparently related to its pe…

astro-ph.SR2010

tau Sco: The discovery of the clones

V. Petit, D. L. Massa, W. L. F. Marcolino +3

The B0.2 V magnetic star tau Sco stands out from the larger population of massive magnetic OB stars due to its remarkable, superionized wind, apparently related to its peculiar mag…

astro-ph.SR2010★ 4 cited

Is the Wind of the Galactic Oe Star HD 155806 Magnetically Confined?

A. W. Fullerton, V. Petit, S. Bagnulo +2

Spectropolarimetric observations of HD 155806 - the hottest Galactic Oe star - were obtained with CFHT/ESPaDOnS to test the hypothesis that disk signatures in its spectrum are due…

astro-ph.SR2010

Modeling the Magnetosphere of the B2Vp star sigma Ori E

M. E. Oksala, G. A. Wade, R. H. D Townsend +2

This paper presents results obtained from Stokes I and V spectra of the B2Vp star sigma Ori E, observed by both the Narval and ESPaDOnS spectropolarimeters. Using Least- Squares De…

astro-ph.SR2010★ 4 cited

The constant magnetic field of xi 1 CMa: geometry or slow rotation?

C. Fourtune-Ravard, G. A. Wade, W. Marcolino +4

We report recent observations of the sharp-lined magnetic beta Cep pulsator xi 1 CMa (= HD 46328). The longitudinal magnetic field of this star is detected consistently, but it is…