The neutral gas in the environs of the Geminga gamma-ray pulsar
暂无分享,去创建一个
Australia. | E. Reynoso | G. Dubner | W. Goss | A. Green | E. Giacani | S. J. Iafe | A. Nrao | Usa Univ. of Sydney
[1] E. Reynoso,et al. Influence of the Neutron Star 1E 161348–5055 in RCW 103 on the Surrounding Medium , 2003, Publications of the Astronomical Society of Australia.
[2] G. Bignami,et al. Geminga's Tails: A Pulsar Bow Shock Probing the Interstellar Medium , 2003, Science.
[3] Iafe,et al. Observations of the neutral hydrogen surrounding the radio-quiet neutron star RX J0822–4300 in Puppis A , 2003, astro-ph/0307065.
[4] D. Frail,et al. Pulsar Wind Nebulae around the Southern Pulsars PSR B1643−43 and PSR B1706−44 , 2001, astro-ph/0103089.
[5] T. Lazio,et al. Upper Limits on the Continuum Emission from Geminga at 74 and 326 MHz , 1999, The Astrophysical journal.
[6] V. D. Pugachev,et al. The radio pulsar Geminga , 1998 .
[7] V. Malofeev,et al. Detection of Geminga as a radio pulsar , 1997, Nature.
[8] Patrizia A. Caraveo,et al. Parallax Observations with the Hubble Space Telescope Yield the Distance to Geminga , 1996 .
[9] D. L. Bertsch,et al. Pulsed high-energy γ-radiation from Geminga (1E0630+178) , 1992, Nature.
[10] G. Dubner,et al. The Interstellar Matter in the Direction of the Supernova Remnant G296.5+10.0 and the Central X-Ray Source 1E 1207.4−5209 , 2000 .
[11] R. Haynes,et al. Southern H II regions: an extensive study of radio recombination line emission , 1987 .