Identification of the fast, high galactic latitude X-ray transient A 0000 + 28 with the RS CVn system HD 224085

D. A. Schwartz; M. Garcia; E. Ralph; R. E. Doxsey; M. D. Johnston; A. Lawrence; I. M. McHardy; J. P. Pye

doi:10.1093/mnras/196.2.95

Identification of the fast, high galactic latitude X-ray transient A 0000 + 28 with the RS CVn system HD 224085

D. A. Schwartz, M. Garcia, E. Ralph, R. E. Doxsey, M. D. Johnston, A. Lawrence, I. M. McHardy, J. P. Pye

School of Physics and Astronomy

Research output: Contribution to journal › Article › peer-review

Abstract

We identify the fast, high galactic latitude X-ray transient A 0000+28 (=3A 2355+284) with HD 224085, a known RSCVn system. This strengthens the suggestion that RS CVn systems are responsible for a significant fraction of this class of X-ray transient. The hard X-ray flares provide further data relevant to the interpretation of these systems by analogy to solar phenomena.

Original language	English
Pages (from-to)	95-100
Journal	Monthly Notices of the Royal Astronomical Society
Volume	196
DOIs	https://doi.org/10.1093/mnras/196.2.95
Publication status	Published - 1 Jul 1981

Keywords / Materials (for Non-textual outputs)

Flare Stars
Stellar Luminosity
Stellar Radiation
X Ray Sources
Ariel 5 Satellite
Binary Stars
Light Curve
Stellar Coronas
X Ray Stars

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10.1093/mnras/196.2.95

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title = "Identification of the fast, high galactic latitude X-ray transient A 0000 + 28 with the RS CVn system HD 224085",

abstract = "We identify the fast, high galactic latitude X-ray transient A 0000+28 (=3A 2355+284) with HD 224085, a known RSCVn system. This strengthens the suggestion that RS CVn systems are responsible for a significant fraction of this class of X-ray transient. The hard X-ray flares provide further data relevant to the interpretation of these systems by analogy to solar phenomena.",

keywords = "Flare Stars, Stellar Luminosity, Stellar Radiation, X Ray Sources, Ariel 5 Satellite, Binary Stars, Light Curve, Stellar Coronas, X Ray Stars",

author = "Schwartz, {D. A.} and M. Garcia and E. Ralph and Doxsey, {R. E.} and Johnston, {M. D.} and A. Lawrence and McHardy, {I. M.} and Pye, {J. P.}",

year = "1981",

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doi = "10.1093/mnras/196.2.95",

language = "English",

volume = "196",

pages = "95--100",

journal = "Monthly Notices of the Royal Astronomical Society",

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publisher = "Oxford University Press",

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TY - JOUR

T1 - Identification of the fast, high galactic latitude X-ray transient A 0000 + 28 with the RS CVn system HD 224085

AU - Schwartz, D. A.

AU - Garcia, M.

AU - Ralph, E.

AU - Doxsey, R. E.

AU - Johnston, M. D.

AU - Lawrence, A.

AU - McHardy, I. M.

AU - Pye, J. P.

PY - 1981/7/1

Y1 - 1981/7/1

N2 - We identify the fast, high galactic latitude X-ray transient A 0000+28 (=3A 2355+284) with HD 224085, a known RSCVn system. This strengthens the suggestion that RS CVn systems are responsible for a significant fraction of this class of X-ray transient. The hard X-ray flares provide further data relevant to the interpretation of these systems by analogy to solar phenomena.

AB - We identify the fast, high galactic latitude X-ray transient A 0000+28 (=3A 2355+284) with HD 224085, a known RSCVn system. This strengthens the suggestion that RS CVn systems are responsible for a significant fraction of this class of X-ray transient. The hard X-ray flares provide further data relevant to the interpretation of these systems by analogy to solar phenomena.

KW - Flare Stars

KW - Stellar Luminosity

KW - Stellar Radiation

KW - X Ray Sources

KW - Ariel 5 Satellite

KW - Binary Stars

KW - Light Curve

KW - Stellar Coronas

KW - X Ray Stars

U2 - 10.1093/mnras/196.2.95

DO - 10.1093/mnras/196.2.95

M3 - Article

SN - 0035-8711

VL - 196

SP - 95

EP - 100

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

ER -

Identification of the fast, high galactic latitude X-ray transient A 0000 + 28 with the RS CVn system HD 224085

Abstract

Keywords / Materials (for Non-textual outputs)

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