Standard

Massive Stars and Black Holes. / Kholtygin, A.F.

In: Publications of the Astronomical Society of the Pacific, Vol. 494, 2015, p. 255-257.

Research output: Contribution to journal › Article

Harvard

Kholtygin, AF 2015, 'Massive Stars and Black Holes', Publications of the Astronomical Society of the Pacific, vol. 494, pp. 255-257. <http://adsabs.harvard.edu/abs/2015ASPC..494..255K>

APA

Kholtygin, A. F. (2015). Massive Stars and Black Holes. Publications of the Astronomical Society of the Pacific, 494, 255-257. http://adsabs.harvard.edu/abs/2015ASPC..494..255K

Vancouver

Kholtygin AF. Massive Stars and Black Holes. Publications of the Astronomical Society of the Pacific. 2015;494:255-257.

Author

Kholtygin, A.F. / Massive Stars and Black Holes. In: Publications of the Astronomical Society of the Pacific. 2015 ; Vol. 494. pp. 255-257.

BibTeX

@article{0de3428493c94752b9daf69ef541c5a9,
title = "Massive Stars and Black Holes",
abstract = "We model the mass distribution of newborn black holes (BHs) using a new population synthesis code for massive stars in the Milky Way. The calculated distributions agree well with those obtained for the galactic BHs in binary systems. The explosions of Wolf–Rayet (WR) precursors may be responsible for the origin of BHs.",
keywords = "звезды, конечные стадии эволюции звезд, xthyst lshs",
author = "A.F. Kholtygin",
year = "2015",
language = "English",
volume = "494",
pages = "255--257",
journal = "Publications of the Astronomical Society of the Pacific",
issn = "0004-6280",
publisher = "University of Chicago Press",

}

RIS

TY - JOUR

T1 - Massive Stars and Black Holes

AU - Kholtygin, A.F.

PY - 2015

Y1 - 2015

N2 - We model the mass distribution of newborn black holes (BHs) using a new population synthesis code for massive stars in the Milky Way. The calculated distributions agree well with those obtained for the galactic BHs in binary systems. The explosions of Wolf–Rayet (WR) precursors may be responsible for the origin of BHs.

AB - We model the mass distribution of newborn black holes (BHs) using a new population synthesis code for massive stars in the Milky Way. The calculated distributions agree well with those obtained for the galactic BHs in binary systems. The explosions of Wolf–Rayet (WR) precursors may be responsible for the origin of BHs.

KW - звезды

KW - конечные стадии эволюции звезд

KW - xthyst lshs

M3 - Article

VL - 494

SP - 255

EP - 257

JO - Publications of the Astronomical Society of the Pacific

JF - Publications of the Astronomical Society of the Pacific

SN - 0004-6280

ER -

ID: 5790066