Standard
Evolution of Neutron Stars in the Milky Way. / Schislyaeva, Y.; Kholtygin, A.; Igoshev, A.
Physics of Magnetic Stars: Proceedings of a Conference Held at Special Astrophysical Observatory, Nizhny Arkhyz, Russia, 1-5 October 2018. ред. / I.I. Romanyuk; I. A. Yakunin; D.O. Kudryavtsev. San Francisco : Astronomical Society of the Pacific, 2019. стр. 111-113 (Astronomical Society of the Pacific conference series; Том 518).
Результаты исследований: Публикации в книгах, отчётах, сборниках, трудах конференций › статья в сборнике материалов конференции › научная
Harvard
Schislyaeva, Y, Kholtygin, A & Igoshev, A 2019,
Evolution of Neutron Stars in the Milky Way. в II Romanyuk, IA Yakunin & DO Kudryavtsev (ред.),
Physics of Magnetic Stars: Proceedings of a Conference Held at Special Astrophysical Observatory, Nizhny Arkhyz, Russia, 1-5 October 2018. Astronomical Society of the Pacific conference series, Том. 518, Astronomical Society of the Pacific, San Francisco, стр. 111-113, International Conference "Physics of Magnetic Stars", Nizhny Arkhyz, Российская Федерация,
1/10/19. <
http://aspbooks.org/custom/publications/paper/518-0111.html>
APA
Schislyaeva, Y., Kholtygin, A., & Igoshev, A. (2019).
Evolution of Neutron Stars in the Milky Way. в I. I. Romanyuk, I. A. Yakunin, & D. O. Kudryavtsev (Ред.),
Physics of Magnetic Stars: Proceedings of a Conference Held at Special Astrophysical Observatory, Nizhny Arkhyz, Russia, 1-5 October 2018 (стр. 111-113). (Astronomical Society of the Pacific conference series; Том 518). Astronomical Society of the Pacific.
http://aspbooks.org/custom/publications/paper/518-0111.html
Vancouver
Schislyaeva Y, Kholtygin A, Igoshev A.
Evolution of Neutron Stars in the Milky Way. в Romanyuk II, Yakunin IA, Kudryavtsev DO, Редакторы, Physics of Magnetic Stars: Proceedings of a Conference Held at Special Astrophysical Observatory, Nizhny Arkhyz, Russia, 1-5 October 2018. San Francisco: Astronomical Society of the Pacific. 2019. стр. 111-113. (Astronomical Society of the Pacific conference series).
Author
Schislyaeva, Y. ; Kholtygin, A. ; Igoshev, A. /
Evolution of Neutron Stars in the Milky Way. Physics of Magnetic Stars: Proceedings of a Conference Held at Special Astrophysical Observatory, Nizhny Arkhyz, Russia, 1-5 October 2018. Редактор / I.I. Romanyuk ; I. A. Yakunin ; D.O. Kudryavtsev. San Francisco : Astronomical Society of the Pacific, 2019. стр. 111-113 (Astronomical Society of the Pacific conference series).
BibTeX
@inproceedings{e5cc4410039446d48857cf8084319943,
title = "Evolution of Neutron Stars in the Milky Way",
abstract = "The present paper is devoted to the analysis of the evolution of young neutron stars (NSs) in the Milky Way up to the death line. The methods of population synthesis have been used to study the distribution of an ensemble of young NSs by their periods, period derivatives, and magnetic fields. The distribution of the initial periods and magnetic fields of the ensemble is assumed to be bimodal. Relatively slowly rotating NSs with initial periods P0{\~ } 1 s become magnetars, whereas NSs with P0{\~ } 300 ms turn into normal pulsars. The model distributions of young NSs by rotation periods, period derivatives, and magnetic fields are compared with those obtained from the ATNF catalog. The location of the model ensemble of NSs on the P-Ṗ diagram appears to be close to the position of the real ensemble of NSs.",
author = "Y. Schislyaeva and A. Kholtygin and A. Igoshev",
year = "2019",
month = jul,
day = "1",
language = "English",
isbn = "9781583819234",
series = "Astronomical Society of the Pacific conference series",
publisher = "Astronomical Society of the Pacific",
pages = "111--113",
editor = "I.I. Romanyuk and Yakunin, {I. A.} and D.O. Kudryavtsev",
booktitle = "Physics of Magnetic Stars",
address = "United States",
note = "International Conference {"}Physics of Magnetic Stars{"} ; Conference date: 01-10-2019 Through 05-10-2019",
}
RIS
TY - GEN
T1 - Evolution of Neutron Stars in the Milky Way
AU - Schislyaeva, Y.
AU - Kholtygin, A.
AU - Igoshev, A.
PY - 2019/7/1
Y1 - 2019/7/1
N2 - The present paper is devoted to the analysis of the evolution of young neutron stars (NSs) in the Milky Way up to the death line. The methods of population synthesis have been used to study the distribution of an ensemble of young NSs by their periods, period derivatives, and magnetic fields. The distribution of the initial periods and magnetic fields of the ensemble is assumed to be bimodal. Relatively slowly rotating NSs with initial periods P0 ̃ 1 s become magnetars, whereas NSs with P0 ̃ 300 ms turn into normal pulsars. The model distributions of young NSs by rotation periods, period derivatives, and magnetic fields are compared with those obtained from the ATNF catalog. The location of the model ensemble of NSs on the P-Ṗ diagram appears to be close to the position of the real ensemble of NSs.
AB - The present paper is devoted to the analysis of the evolution of young neutron stars (NSs) in the Milky Way up to the death line. The methods of population synthesis have been used to study the distribution of an ensemble of young NSs by their periods, period derivatives, and magnetic fields. The distribution of the initial periods and magnetic fields of the ensemble is assumed to be bimodal. Relatively slowly rotating NSs with initial periods P0 ̃ 1 s become magnetars, whereas NSs with P0 ̃ 300 ms turn into normal pulsars. The model distributions of young NSs by rotation periods, period derivatives, and magnetic fields are compared with those obtained from the ATNF catalog. The location of the model ensemble of NSs on the P-Ṗ diagram appears to be close to the position of the real ensemble of NSs.
UR - https://catalog.princeton.edu/catalog/11469461
M3 - Conference contribution
SN - 9781583819234
T3 - Astronomical Society of the Pacific conference series
SP - 111
EP - 113
BT - Physics of Magnetic Stars
A2 - Romanyuk, I.I.
A2 - Yakunin, I. A.
A2 - Kudryavtsev, D.O.
PB - Astronomical Society of the Pacific
CY - San Francisco
T2 - International Conference "Physics of Magnetic Stars"
Y2 - 1 October 2019 through 5 October 2019
ER -
