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Dynamical mass of the O-type supergiant inζOrionis A

author

Otmar Stahl

published in: Astronomy and Astrophysics

date of publication: 2013-06

language: English

Cites articles 16

Date

Title

Authors

2013-01-18

Temperature, gravity, and bolometric correction scales for non-supergiant OB stars
2011-05-23

Rotating massive main-sequence stars

Matteo Cantiello, Selma E. de Mink, Alex de Koter
2009-10-07

Accurate masses and radii of normal stars: modern results and applications
2009-02-09

Tracing the young massive high-eccentricity binary system $\theta^{\mathsf 1}$Orionis C through periastron passage

Stefan Kraus
2009-09-15

The interstellar Ca II distance scale
2007

Validation of the new Hipparcos reduction

Floor van Leeuwen
2007-08-28

The distance to the Orion Nebula

Karl Martin Menten, Andreas Brunthaler
2006-06

A high-resolution spectroscopy survey of β Cephei pulsations in bright stars
2004-11-23

On the Hipparcos parallaxes of O stars

Anthony G.A. Brown
2003-05

First Observations with a Co-phased Six-Station Optical Long-Baseline Array: Application to the Triple Star Virginis
2000-09-10

ζ Orionis A is a Double Star
1998-05

$uvby\beta$ photoelectric photometric catalogue
1998-03-20

The Navy Prototype Optical Interferometer
1996-09

Transformations from Theoretical Hertzsprung-Russell Diagrams to Color-Magnitude Diagrams: Effective Temperatures, B-V Colors, and Bolometric Corrections
1976-04

MK classification for visual binary components
1974-04-01

The Angular Diameters of 32 Stars

Article - wd:Q53998171

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