1932

Annual Review of Astronomy and Astrophysics

Volume 31, 1993

Review Article

Origin and Evolution of X-Ray Binaries and Binary Radio Pulsars

Frank Verbunt
Vol. 31:93-127 (Volume publication date September 1993) https://doi.org/10.1146/annurev.aa.31.090193.000521
© Annual Reviews

There is no abstract available.

Keyword(s): black holes, mass exchange, mass loss, neutron stars, Roche lobe, spiral-in

Article metrics loading...

/content/journals/10.1146/annurev.aa.31.090193.000521

1993-09-01

2024-12-02

Loading full text...

Full text loading...

/content/journals/10.1146/annurev.aa.31.090193.000521

Article Type: Review Article

Most Cited Most Cited RSS feed

- The Chemical Composition of the Sun
  
  Martin Asplund, Nicolas Grevesse, A. Jacques Sauval, and Pat Scott
  
  Vol. 47 (2009), pp. 481–522
- STAR FORMATION IN GALAXIES ALONG THE HUBBLE SEQUENCE
  
  Robert C. Kennicutt Jr.
  
  Vol. 36 (1998), pp. 189–231
- Smoothed Particle Hydrodynamics
  
  J. J. Monaghan
  
  Vol. 30 (1992), pp. 543–574
- H I in the Galaxy
  
  John M. Dickey, and Felix J. Lockman
  
  Vol. 28 (1990), pp. 215–259
- Unified Models for Active Galactic Nuclei and Quasars
  
  Robert Antonucci
  
  Vol. 31 (1993), pp. 473–521
- Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
  
  John Kormendy, and Luis C. Ho
  
  Vol. 51 (2013), pp. 511–653
- Cosmic Star-Formation History
  
  Piero Madau, and Mark Dickinson
  
  Vol. 52 (2014), pp. 415–486
- Embedded Clusters in Molecular Clouds
  
  Charles J. Lada, and Elizabeth A. Lada
  
  Vol. 41 (2003), pp. 57–115
- LUMINOUS INFRARED GALAXIES
  
  D. B. Sanders, and I. F. Mirabel
  
  Vol. 34 (1996), pp. 749–792
- Star Formation in the Milky Way and Nearby Galaxies
  
  Robert C. Kennicutt Jr., and Neal J. Evans II
  
  Vol. 50 (2012), pp. 531–608
More Less

This is a required field

Please enter a valid email address

Approval was a Success

Invalid data

An Error Occurred

Approval was partially successful, following selected items could not be processed due to error