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Titolo:
THE PROPER MOTION AND WIND NEBULA OF THE NEARBY MILLISECOND PULSAR J0437-4715
Autore:
BELL JF; BAILES M; MANCHESTER RN; WEISBERG JM; LYNE AG;
Indirizzi:
AUSTRALIAN NATL UNIV,MT STROMLO & SIDING SPRING OBSERV,INST ADV STUDIES WESTON ACT 2611 AUSTRALIA CSIRO,AUSTRALIA TELESCOPE NATL FACIL EPPING NSW 2121 AUSTRALIA CARLETON COLL,DEPT PHYS & ASTRON NORTHFIELD MN 55057 UNIV MANCHESTER,NUFFIELD RADIO ASTRON LABS,JODRELL BANK MACCLESFIELD SK11 9DL CHESHIRE ENGLAND
Titolo Testata:
The Astrophysical journal
fascicolo: 2, volume: 440, anno: 1995,
parte:, 2
pagine: 81 - 83
SICI:
0004-637X(1995)440:2<81:TPMAWN>2.0.ZU;2-P
Fonte:
ISI
Lingua:
ENG
Soggetto:
OPTICAL SPECTROSCOPY; BOW-SHOCK; PSR 1957; COMPANION; BRIGHT; ASTROMETRY; EVOLUTION; SYSTEM;
Keywords:
ISM, H II REGIONS; PULSARS, INDIVIDUAL (PSR J0437 -4715);
Tipo documento:
Article
Natura:
Periodico
Settore Disciplinare:
Science Citation Index Expanded
Citazioni:
21
Recensione:
Indirizzi per estratti:
Citazione:
J.F. Bell et al., "THE PROPER MOTION AND WIND NEBULA OF THE NEARBY MILLISECOND PULSAR J0437-4715", The Astrophysical journal, 440(2), 1995, pp. 81-83

Abstract

Pulse arrival time measurements have been obtained over a 2 year interval for PSR J0437-4715 using the Parkes radio telescope. These data show that the proper motion of the pulsar is 135 +/- 4 mas yr(-1) at a position angle of 122 degrees +/- 2 degrees. This agrees well with theproper motion of the optical companion, putting the association beyond doubt. An H alpha image confirms that the nebulosity first detected by Bell, Bailes, and Bessell is a bow shock associated with the pulsarand shows that its orientation is close to that expected from the proper motion.

ASDD Area Sistemi Dipartimentali e Documentali, Università di Bologna, Catalogo delle riviste ed altri periodici
Documento generato il 20/06/13 alle ore 09:42:14