WHT observations of cataclysmic variables in globular clusters - III. V4 in M30 during quiescence

G. Machin; J. Allington-Smith; P. J. Callanan; P. A. Charles; B. J.M. Hassall; K. O. Mason; K. Mukai; T. Naylor; A. P. Smale; J. Van Paradijs

doi:10.1093/mnras/250.3.602

WHT observations of cataclysmic variables in globular clusters - III. V4 in M30 during quiescence

G. Machin
, J. Allington-Smith
, P. J. Callanan
, P. A. Charles
, B. J.M. Hassall
, K. O. Mason
, K. Mukai
, T. Naylor
, A. P. Smale
, J. Van Paradijs

University of Oxford
National Physical Laboratory
Durham University
Royal Observatory, Greenwich
University College London
University of California at Berkeley
University of Cambridge
NASA Goddard Space Flight Center
University of Amsterdam
NIKHEFH

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

Abstract

We report the results of William Herschel telescope (WHT) observations of the candidate globular-cluster dwarf nova, V4 in M30. We find that, on the basis of its quiescent magnitude and colours, its outburst magnitude and its radial velocity, V4 is likely to be a foreground object in the field of M30. In addition, it is probably a shortperiod system near the period gap.

Original language	English
Pages (from-to)	602-606
Number of pages	5
Journal	Monthly Notices of the Royal Astronomical Society
Volume	250
Issue number	3
DOIs	https://doi.org/10.1093/mnras/250.3.602
Publication status	Published - 1991
Externally published	Yes

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10.1093/mnras/250.3.602

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@article{a801430e26e04f3ba9521e2298638084,

title = "WHT observations of cataclysmic variables in globular clusters - III. V4 in M30 during quiescence",

abstract = "We report the results of William Herschel telescope (WHT) observations of the candidate globular-cluster dwarf nova, V4 in M30. We find that, on the basis of its quiescent magnitude and colours, its outburst magnitude and its radial velocity, V4 is likely to be a foreground object in the field of M30. In addition, it is probably a shortperiod system near the period gap.",

author = "G. Machin and J. Allington-Smith and Callanan, \{P. J.\} and Charles, \{P. A.\} and Hassall, \{B. J.M.\} and Mason, \{K. O.\} and K. Mukai and T. Naylor and Smale, \{A. P.\} and \{Van Paradijs\}, J.",

note = "Publisher Copyright: {\textcopyright} Royal Astronomical Society. Provided by the NASA Astrophysics Data System.",

year = "1991",

doi = "10.1093/mnras/250.3.602",

language = "English",

volume = "250",

pages = "602--606",

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

issn = "0035-8711",

publisher = "Oxford University Press",

number = "3",

}

TY - JOUR

T1 - WHT observations of cataclysmic variables in globular clusters - III. V4 in M30 during quiescence

AU - Machin, G.

AU - Allington-Smith, J.

AU - Callanan, P. J.

AU - Charles, P. A.

AU - Hassall, B. J.M.

AU - Mason, K. O.

AU - Mukai, K.

AU - Naylor, T.

AU - Smale, A. P.

AU - Van Paradijs, J.

PY - 1991

Y1 - 1991

N2 - We report the results of William Herschel telescope (WHT) observations of the candidate globular-cluster dwarf nova, V4 in M30. We find that, on the basis of its quiescent magnitude and colours, its outburst magnitude and its radial velocity, V4 is likely to be a foreground object in the field of M30. In addition, it is probably a shortperiod system near the period gap.

AB - We report the results of William Herschel telescope (WHT) observations of the candidate globular-cluster dwarf nova, V4 in M30. We find that, on the basis of its quiescent magnitude and colours, its outburst magnitude and its radial velocity, V4 is likely to be a foreground object in the field of M30. In addition, it is probably a shortperiod system near the period gap.

UR - https://www.scopus.com/pages/publications/4243361568

U2 - 10.1093/mnras/250.3.602

DO - 10.1093/mnras/250.3.602

M3 - Article

AN - SCOPUS:4243361568

SN - 0035-8711

VL - 250

SP - 602

EP - 606

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 3

ER -

WHT observations of cataclysmic variables in globular clusters - III. V4 in M30 during quiescence

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