Time-resolved optical observations of PSR 1509-58

A. Shearer; C. M.M. O' Sullivan; A. Golden; P. V.R. Garcia; M. Redfern; A. Danks; M. Cullum

Time-resolved optical observations of PSR 1509-58

A. Shearer
, C. M.M. O' Sullivan
, A. Golden
, P. V.R. Garcia
, M. Redfern
, A. Danks
, M. Cullum

Physics

Research output: Contribution to a Journal (Peer & Non Peer) › Review article › peer-review

2 Citations (Scopus)

Abstract

Using time resolved 2-dimensional aperture photometry we have established that the optical candidate for PSR 1509-58 does not pulse. Our pulsed upper limits (m_V = 24.3 and m_B = 25.7) put severe constraints on this being the optical counterpart. Furthermore the colours of the candidate star are consistent with a main sequence star at a distance of 2-4 kpc. The probability of a chance coincidence with a normal star and the difficulty of explaining the lack of pulsed emission leads us to conclude that this object is an intermediate field star.

Original language	English
Pages (from-to)	l-16l18
Journal	Astronomy and Astrophysics
Volume	333
Issue number	1
Publication status	Published - 1998

Keywords

Pulsars: individual: PSR 1509-58

Cite this

@article{11e3a7f8368f4eeebfda636a0e6decde,

title = "Time-resolved optical observations of PSR 1509-58",

abstract = "Using time resolved 2-dimensional aperture photometry we have established that the optical candidate for PSR 1509-58 does not pulse. Our pulsed upper limits (mV = 24.3 and mB = 25.7) put severe constraints on this being the optical counterpart. Furthermore the colours of the candidate star are consistent with a main sequence star at a distance of 2-4 kpc. The probability of a chance coincidence with a normal star and the difficulty of explaining the lack of pulsed emission leads us to conclude that this object is an intermediate field star.",

keywords = "Pulsars: individual: PSR 1509-58",

author = "A. Shearer and \{O' Sullivan\}, \{C. M.M.\} and A. Golden and Garcia, \{P. V.R.\} and M. Redfern and A. Danks and M. Cullum",

year = "1998",

language = "English",

volume = "333",

pages = "l--16l18",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

number = "1",

}

TY - JOUR

T1 - Time-resolved optical observations of PSR 1509-58

AU - Shearer, A.

AU - O' Sullivan, C. M.M.

AU - Golden, A.

AU - Garcia, P. V.R.

AU - Redfern, M.

AU - Danks, A.

AU - Cullum, M.

PY - 1998

Y1 - 1998

N2 - Using time resolved 2-dimensional aperture photometry we have established that the optical candidate for PSR 1509-58 does not pulse. Our pulsed upper limits (mV = 24.3 and mB = 25.7) put severe constraints on this being the optical counterpart. Furthermore the colours of the candidate star are consistent with a main sequence star at a distance of 2-4 kpc. The probability of a chance coincidence with a normal star and the difficulty of explaining the lack of pulsed emission leads us to conclude that this object is an intermediate field star.

AB - Using time resolved 2-dimensional aperture photometry we have established that the optical candidate for PSR 1509-58 does not pulse. Our pulsed upper limits (mV = 24.3 and mB = 25.7) put severe constraints on this being the optical counterpart. Furthermore the colours of the candidate star are consistent with a main sequence star at a distance of 2-4 kpc. The probability of a chance coincidence with a normal star and the difficulty of explaining the lack of pulsed emission leads us to conclude that this object is an intermediate field star.

KW - Pulsars: individual: PSR 1509-58

UR - https://www.scopus.com/pages/publications/0040037803

M3 - Review article

SN - 0004-6361

VL - 333

SP - l-16l18

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

IS - 1

ER -

Time-resolved optical observations of PSR 1509-58

Abstract

Keywords

Other files and links

Fingerprint

Cite this