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Ionizing spectra of stars that lose their envelope through interaction with a binary companion: role of metallicity

Ionizing spectra of stars that lose their envelope through interaction with a binary companion: role of metallicity

http://www.wikidata.org/entity/Q59093171

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Ionizing spectra of stars that lose their envelope through interaction with a binary companion: role of metallicity

http://www.wikidata.org/entity/Q59093171

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article publié dans la revue scientifique Astronomy and Astrophysics

@fr

im November 2017 veröffentlichter wissenschaftlicher Artikel

@de

scientific article published in Astronomy and Astrophysics

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wetenschappelijk artikel

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наукова стаття, опублікована в листопаді 2017

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name

Ionizing spectra of stars that ...... companion: role of metallicity

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Ionizing spectra of stars that ...... companion: role of metallicity

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type

label

Ionizing spectra of stars that ...... companion: role of metallicity

@en

Ionizing spectra of stars that ...... companion: role of metallicity

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Ionizing spectra of stars that ...... companion: role of metallicity

@en

Ionizing spectra of stars that ...... companion: role of metallicity

@nl

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Astronomy and Astrophysics

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Ionizing spectra of stars that ...... companion: role of metallicity

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P2093

J. H. Groh

http://www.w3.org/2001/XMLSchema#string

S. E. de Mink

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Y. Götberg

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P2860

THE EXTENDED He II λ 4686-EMITTING REGION IN IZw 18 UNVEILED: CLUES FOR PECULIAR IONIZING SOURCES

The Luminosity Function and Stellar Evolution.

Evolutionary tracks and isochrones for low- and intermediate-mass stars: From 0.15 to 7 M?, and from Z=0.0004 to 0.03

Theoretical Modeling of Starburst Galaxies

The VLT-FLAMES Tarantula Survey

Binary interaction dominates the evolution of massive stars.

The first gravitational-wave source from the isolated evolution of two stars in the 40-100 solar mass range.

Formation of the first three gravitational-wave observations through isolated binary evolution

The evolution of massive stars and their spectra. I. A non-rotating 60 M_{sun}_ star from the zero-age main sequence to the pre-supernova stage

A spectroscopic survey on the multiplicity of high-mass stars

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11–11

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scholarly article

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10.1051/0004-6361/201730472

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P478

608

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2017-11-29T00:00:00Z

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1701.07439

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P819

2017A&A...608A..11G

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