(Q54257502)

2

object named as

H. F. Henrichs

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author name string

R. S. Schnerr

1

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E. Verdugo

4

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J. de Jong

5

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V. C. Geers

6

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K. Wiersema

7

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B. van Dalen

8

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A. Tijani

9

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B. Plaggenborg

10

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K. L. J. Rygl

Astronomy and Astrophysics

11

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language of work or name

English

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publication date

26 March 2008

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published in

1 reference

SIMBAD

volume

483

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SIMBAD

issue

3

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page(s)

857–867

1 reference

The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars

SIMBAD

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1 reference

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Mitteilung über veränderliche Sterne

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A fossil origin for the magnetic field in A stars and white dwarfs

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Physical parameters and wind properties of galactic early B supergiants

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The surprising magnetic topology of Sco: fossil remnant or dynamo output?

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Carbon, nitrogen, and oxygen abundances in early B-type stars

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New periodic variables from the Hipparcos epoch photometry

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Surface abundances of light elements for a large sample of early B-type stars – III. An analysis of helium lines in spectra of 102 stars

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Spectral variability of luminous early type stars. II. Supergiant {alpha} Camelopardalis

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Large-scale wind structures in OB supergiants: a search for rotationally modulated H variability

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Discovery of a magnetic field in the Slowly Pulsating B star $\zeta$ Cassiopeiae

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Metallicities of the SPB stars from the IUE ultraviolet spectra

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Chemical composition of Galactic OB stars

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Magnetism in Isolated and Binary White Dwarfs

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Discovery of magnetic fields in the Cephei star 1 CMa and in several slowly pulsating B stars

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Elemental abundance analyses with DAO spectrograms. XXIX. The mercury-manganese stars 53 Tau, β Tau, γ Crv, and υ Her

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Catalogue of averaged stellar effective magnetic fields. I. Chemically peculiar A and B type stars

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Spectral analysis of early-type stars using a genetic algorithm based fitting method

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Contemporary optical spectral classification of the OB stars - A digital atlas

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N-body simulations of stars escaping from the Orion nebula

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The magnetic field and wind confinement ofθ1Orionis C

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Discovery of a strong magnetic field on the O star HD 191612: new clues to the future of 1 Orionis C

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Dynamical Simulations of Magnetically Channeled Line‐driven Stellar Winds. I. Isothermal, Nonrotating, Radially Driven Flow

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Observations of Magnetic Fields on T Tauri Stars

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