IR contamination in quiescence X-Ray Novae

Mark T. Reynolds; Paul J. Callanan; Colm Kelleher

doi:10.1017/S1743921307005820

IR contamination in quiescence X-Ray Novae

Mark T. Reynolds
, Paul J. Callanan
, Colm Kelleher

School of Physics

University College Cork

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

Abstract

We present archival optical-IR observations of a number of short period X-ray novae (XRNe). We use these to show that in contrast to the current paradigm, there is likely significant non stellar flux in the infra-red (IR).

Original language	English
Pages (from-to)	435-436
Number of pages	2
Journal	Proceedings of the International Astronomical Union
Volume	2
Issue number	S238
DOIs	https://doi.org/10.1017/S1743921307005820
Publication status	Published - Aug 2006

Keywords

Stars: individual (XTE J1118+480, GRO J0422+32, A0620-00, GS2000+25, GS1142-68 & Cen X-4)
X-rays: binaries

Access to Document

10.1017/S1743921307005820

Cite this

@article{60162e7816ab4752b2535a5a0f4009b7,

title = "IR contamination in quiescence X-Ray Novae",

abstract = "We present archival optical-IR observations of a number of short period X-ray novae (XRNe). We use these to show that in contrast to the current paradigm, there is likely significant non stellar flux in the infra-red (IR).",

keywords = "Stars: individual (XTE J1118+480, GRO J0422+32, A0620-00, GS2000+25, GS1142-68 \& Cen X-4), X-rays: binaries",

author = "Reynolds, \{Mark T.\} and Callanan, \{Paul J.\} and Colm Kelleher",

year = "2006",

month = aug,

doi = "10.1017/S1743921307005820",

language = "English",

volume = "2",

pages = "435--436",

journal = "Proceedings of the International Astronomical Union",

issn = "1743-9213",

publisher = "Cambridge University Press",

number = "S238",

}

TY - JOUR

T1 - IR contamination in quiescence X-Ray Novae

AU - Reynolds, Mark T.

AU - Callanan, Paul J.

AU - Kelleher, Colm

PY - 2006/8

Y1 - 2006/8

N2 - We present archival optical-IR observations of a number of short period X-ray novae (XRNe). We use these to show that in contrast to the current paradigm, there is likely significant non stellar flux in the infra-red (IR).

AB - We present archival optical-IR observations of a number of short period X-ray novae (XRNe). We use these to show that in contrast to the current paradigm, there is likely significant non stellar flux in the infra-red (IR).

KW - Stars: individual (XTE J1118+480, GRO J0422+32, A0620-00, GS2000+25, GS1142-68 & Cen X-4)

KW - X-rays: binaries

UR - https://www.scopus.com/pages/publications/37049004207

U2 - 10.1017/S1743921307005820

DO - 10.1017/S1743921307005820

M3 - Article

AN - SCOPUS:37049004207

SN - 1743-9213

VL - 2

SP - 435

EP - 436

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

IS - S238

ER -

IR contamination in quiescence X-Ray Novae

Abstract

Keywords

Access to Document

Other files and links

Fingerprint

Cite this