(Q59093168)

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Forming short-period Wolf–Rayet X-ray binaries and double black holes through stable mass transfer

scholarly article by E. P. J. van den Heuvel et al published 26 June 2017 in Monthly Notices of the Royal Astronomical Society

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Forming short-period Wolf–Rayet X-ray binaries and double black holes through stable mass transfer (English)

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3

S. E. de Mink

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author name string

E. P. J. van den Heuvel

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1

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S. F. Portegies Zwart

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2

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language of work or name

English

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publication date

26 June 2017

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number of pages

9 page

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Monthly Notices of the Royal Astronomical Society

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volume

471

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issue

4

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page(s)

4256–4264

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cites work

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

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21 January 2018

A Be-type star with a black-hole companion

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21 January 2018

Physical Properties of Wolf-Rayet Stars

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21 January 2018

Approximations to the radii of Roche lobes

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Grids of stellar models with rotation

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21 January 2018

On the formation and evolution of the first Be star in a black hole binary MWC 656

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21 January 2018

Spectroscopic Observations of the Mass Donor Star in SS 433

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21 January 2018

The luminous blue variables: Astrophysical geysers

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21 January 2018

Comprehensive analytic formulae for stellar evolution as a function of mass and metallicity

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21 January 2018

Common envelope evolution: where we stand and how we can move forward

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21 January 2018

The mass of the black hole in Cygnus X-1

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21 January 2018

Binary interaction dominates the evolution of massive stars.

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21 January 2018

The Galactic WC stars

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21 January 2018

The VIIth catalogue of galactic Wolf–Rayet stars

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21 January 2018

Infrared helium emission lines from Cygnus X-3 suggesting a Wolf-Rayet star companion

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21 January 2018

Identifiers

DOI

10.1093/MNRAS/STX1430

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(Q59093168)

Forming short-period Wolf–Rayet X-ray binaries and double black holes through stable mass transfer

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