✦ LIBER ✦

A systematic study of low-mass X-ray binaries in the M31 globular cluster system

✍ Scribed by Mark B. Peacock; Thomas J. Maccarone; Arunav Kundu; Stephen E. Zepf

Book ID: 110849352
Publisher: John Wiley and Sons
Year: 2010
Tongue: English
Weight: 767 KB
Volume: 407
Category: Article
ISSN: 0035-8711
DOI: 10.1111/j.1365-2966.2010.17119.x

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Wide Field CAMera survey of M31 globular

Wide Field CAMera survey of M31 globular clusters: low-mass X-ray binaries

✍ Mark B. Peacock; Thomas J. Maccarone; Christopher Z. Waters; Arunav Kundu; Steph 📂 Article 📅 2009 🏛 John Wiley and Sons 🌐 English ⚖ 124 KB

Neutron star atmosphere composition: the

Neutron star atmosphere composition: the quiescent, low-mass X-ray binary in the globular cluster M28

✍ M. Servillat; C. O. Heinke; W. C. G. Ho; J. E. Grindlay; J. Hong; M. van den Ber 📂 Article 📅 2012 🏛 John Wiley and Sons 🌐 English ⚖ 515 KB

On the properties of 21 X-ray globular c

On the properties of 21 X-ray globular clusters in M31

✍ P. Battistini; F. Bònoli; R. Buonanno; C. Cacciarl; C. E. Corsi; F. Fusi Pecci 📂 Article 📅 1981 🏛 Springer Netherlands 🌐 English ⚖ 198 KB

The missing link: a low-mass X-ray binar

The missing link: a low-mass X-ray binary in M31 seen as an ultraluminous X-ray source

✍ Matthew J. Middleton; Andrew D. Sutton; Timothy P. Roberts; Floyd E. Jackson; Ch 📂 Article 📅 2012 🏛 John Wiley and Sons 🌐 English ⚖ 559 KB

The luminosity function of low-mass X-ra

The luminosity function of low-mass X-ray binaries in galaxies

✍ K. A. Postnov; A. G. Kuranov 📂 Article 📅 2005 🏛 Springer 🌐 English ⚖ 185 KB

The formation of high-mass black holes i

The formation of high-mass black holes in low-mass X-ray binaries

✍ G.E. Brown; C.-H. Lee; Hans A. Bethe 📂 Article 📅 1999 🏛 Elsevier Science 🌐 English ⚖ 94 KB

We suggest that high-mass black holes; i.e., black holes of several solar masses, can be formed in binaries with low-mass main-sequence companions, provided that the hydrogen envelope of the massive star is removed in common envelope evolution which begins only after the massive star has finished He