Cen X-4 returns to quiescent levels in X-ray, optical, and UV

J. van den Eijnden; Maria Cristina Baglio; J. Homan; Payaswini Saikia; David M. Russell; Stefan Waterval; D. M. Bramich; Fraser Lewis; P. Roche

Cen X-4 returns to quiescent levels in X-ray, optical, and UV

J. van den Eijnden, Maria Cristina Baglio, J. Homan, Payaswini Saikia, David M. Russell, Stefan Waterval, D. M. Bramich, Fraser Lewis, P. Roche

Physics

Research output: Contribution to journal › Article

Abstract

Cen X-4 is a neutron star low-mass X-ray binary located at a close distance of ~1.2 kpc. After its first two outbursts, in 1969 and 1979, it remained in quiescence for more than 40 years.

Original language	English (US)
Journal	The Astronomer's Telegram, No. 14317
Volume	4317
State	Published - Jan 1 2021

Keywords

Neutron Star
Transient

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http://adsabs.harvard.edu/abs/2021ATel14317....1V

Cite this

@article{a74c8b0cbfbf4a9ebcd6521c182e2dc4,

title = "Cen X-4 returns to quiescent levels in X-ray, optical, and UV",

abstract = "Cen X-4 is a neutron star low-mass X-ray binary located at a close distance of ~1.2 kpc. After its first two outbursts, in 1969 and 1979, it remained in quiescence for more than 40 years.",

keywords = "Neutron Star, Transient",

author = "{van den Eijnden}, J. and Baglio, {Maria Cristina} and J. Homan and Payaswini Saikia and Russell, {David M.} and Stefan Waterval and Bramich, {D. M.} and Fraser Lewis and P. Roche",

year = "2021",

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day = "1",

language = "English (US)",

volume = "4317",

journal = "The Astronomer's Telegram, No. 14317",

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TY - JOUR

T1 - Cen X-4 returns to quiescent levels in X-ray, optical, and UV

AU - van den Eijnden, J.

AU - Baglio, Maria Cristina

AU - Homan, J.

AU - Saikia, Payaswini

AU - Russell, David M.

AU - Waterval, Stefan

AU - Bramich, D. M.

AU - Lewis, Fraser

AU - Roche, P.

PY - 2021/1/1

Y1 - 2021/1/1

N2 - Cen X-4 is a neutron star low-mass X-ray binary located at a close distance of ~1.2 kpc. After its first two outbursts, in 1969 and 1979, it remained in quiescence for more than 40 years.

AB - Cen X-4 is a neutron star low-mass X-ray binary located at a close distance of ~1.2 kpc. After its first two outbursts, in 1969 and 1979, it remained in quiescence for more than 40 years.

KW - Neutron Star

KW - Transient

M3 - Article

VL - 4317

JO - The Astronomer's Telegram, No. 14317

JF - The Astronomer's Telegram, No. 14317

ER -

Cen X-4 returns to quiescent levels in X-ray, optical, and UV

Abstract

Keywords

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