Standard

Specific features of the reflection effect in binary systems with compact source rotating about its axis. / Dementyev, A. V.

в: New Astronomy, Том 37, 2015.

Результаты исследований: Научные публикации в периодических изданиях › статья

Harvard

Dementyev, AV 2015, 'Specific features of the reflection effect in binary systems with compact source rotating about its axis', New Astronomy, Том. 37. https://doi.org/10.1016/j.newast.2014.12.002

APA

Dementyev, A. V. (2015). Specific features of the reflection effect in binary systems with compact source rotating about its axis. New Astronomy, 37. https://doi.org/10.1016/j.newast.2014.12.002

Vancouver

Dementyev AV. Specific features of the reflection effect in binary systems with compact source rotating about its axis. New Astronomy. 2015;37. https://doi.org/10.1016/j.newast.2014.12.002

Author

Dementyev, A. V. / Specific features of the reflection effect in binary systems with compact source rotating about its axis. в: New Astronomy. 2015 ; Том 37.

BibTeX

@article{89a066c179b045448c3051e635d996a8,
title = "Specific features of the reflection effect in binary systems with compact source rotating about its axis",
abstract = "Reprocessing of X-ray pulsar radiation by the atmosphere of a companion in a binary system may result in reflected pulse radiation under suitable conditions. In this paper the influence of the rotation of the source of the radiation about its axis on the parameters of thus reflected pulses is investigated. The binary system is modeled by the spherical reflective screen and the compact source uniformly rotating about its axis; the beam pattern (BP) of the source periodically runs along the surface of the screen. Irradiation of the screen by the pulses which have infinitely narrow time spread and by the rectangular pulses is considered. The model does not concern the details of the reprocessing and reemission of the photons. In this model parameters of the pulses reflected in some directions are calculated. The main conclusion provided by the consideration of this model is that the properties of reflected pulses — their profile and observed time of arrival — substantially depend on the correlation between the l",
keywords = "Binaries: close, Pulsars: general, X-rays: binaries",
author = "Dementyev, {A. V.}",
year = "2015",
doi = "10.1016/j.newast.2014.12.002",
language = "English",
volume = "37",
journal = "New Astronomy",
issn = "1384-1092",
publisher = "Elsevier",

}

RIS

TY - JOUR

T1 - Specific features of the reflection effect in binary systems with compact source rotating about its axis

AU - Dementyev, A. V.

PY - 2015

Y1 - 2015

N2 - Reprocessing of X-ray pulsar radiation by the atmosphere of a companion in a binary system may result in reflected pulse radiation under suitable conditions. In this paper the influence of the rotation of the source of the radiation about its axis on the parameters of thus reflected pulses is investigated. The binary system is modeled by the spherical reflective screen and the compact source uniformly rotating about its axis; the beam pattern (BP) of the source periodically runs along the surface of the screen. Irradiation of the screen by the pulses which have infinitely narrow time spread and by the rectangular pulses is considered. The model does not concern the details of the reprocessing and reemission of the photons. In this model parameters of the pulses reflected in some directions are calculated. The main conclusion provided by the consideration of this model is that the properties of reflected pulses — their profile and observed time of arrival — substantially depend on the correlation between the l

AB - Reprocessing of X-ray pulsar radiation by the atmosphere of a companion in a binary system may result in reflected pulse radiation under suitable conditions. In this paper the influence of the rotation of the source of the radiation about its axis on the parameters of thus reflected pulses is investigated. The binary system is modeled by the spherical reflective screen and the compact source uniformly rotating about its axis; the beam pattern (BP) of the source periodically runs along the surface of the screen. Irradiation of the screen by the pulses which have infinitely narrow time spread and by the rectangular pulses is considered. The model does not concern the details of the reprocessing and reemission of the photons. In this model parameters of the pulses reflected in some directions are calculated. The main conclusion provided by the consideration of this model is that the properties of reflected pulses — their profile and observed time of arrival — substantially depend on the correlation between the l

KW - Binaries: close

KW - Pulsars: general

KW - X-rays: binaries

U2 - 10.1016/j.newast.2014.12.002

DO - 10.1016/j.newast.2014.12.002

M3 - Article

VL - 37

JO - New Astronomy

JF - New Astronomy

SN - 1384-1092

ER -

ID: 3924369