A possible optical counterpart to the old nearby pulsar J0108-1431

Astronomy and Astrophysics

Volumn 488, Issue 3, 2008, Pages 1027-1030

  Mignani, R P ^a   Pavlov, G ^b   Kargaltsev, O ^b,c  

^a UNIVERSITY COLLEGE LONDON   (United Kingdom)

^b PENNSYLVANIA STATE UNIVERSITY   (United States)

^c UNIVERSITY OF FLORIDA   (United States)

Author keywords

Astrometry; Stars: pulsars: individual: PSR J0108 1431

Indexed keywords

EMISSION SPECTROSCOPY; IMAGING TECHNIQUES; MAGNETOSPHERE; NEUTRONS; OPTICAL TELESCOPES; PHOTOGRAPHY;

ASTROMETRY; BRIGHTNESS TEMPERATURE; CHANDRA; LONG-TERM EVOLUTION; MULTI-WAVELENGTH STUDY; NEUTRON STARS; NON-THERMAL EMISSION; OPTICAL COUNTERPART; OPTICAL IDENTIFICATION; OPTICAL OBSERVATIONS; PROPER MOTIONS; RADIO PULSARS; STARS: PULSARS: INDIVIDUAL: PSR J0108-1431; VERY LARGE TELESCOPE;

STARS;

EID: 51949116368     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810212     Document Type: Article

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