Zobrazeno 1 - 10
of 24
pro vyhledávání: '"Dubner, G. M."'
Autor:
Bykov, A. M., Krassilchtchikov, A. M., Uvarov, Yu. A., Bloemen, H., Bocchino, F., Dubner, G. M., Giacani, E. B., Pavlov, G. G.
Publikováno v:
The Astrophysical Journal, v. 676, p. 1050-1063, 2008
The nature of the extended hard X-ray source XMMU J061804.3+222732 and its surroundings is investigated using XMM-Newton, Chandra, and Spitzer observations. This source is located in an interaction region of the IC 443 supernova remnant with a neighb
Externí odkaz:
http://arxiv.org/abs/0801.1255
Autor:
Bykov, A. M., Krassilchtchikov, A. M., Uvarov, Yu. A., Kennea, J. A., Pavlov, G. G., Dubner, G. M., Giacani, E. B., Bloemen, H., Hermsen, W., Kaastra, J., Lebrun, F., Renaud, M., Terrier, R., DeBecker, M., Rauw, G., Swings, J. -P.
Publikováno v:
Astrophys.J.649:L21-L24,2006
We found a very likely counterpart to the recently discovered hard X-ray source IGR J2018+4043 in the multi-wavelength observations of the source field. The source, originally discovered in the 20-40 keV band, is now confidently detected also in the
Externí odkaz:
http://arxiv.org/abs/astro-ph/0609676
We have carried out an HI survey towards X-ray central compact objects (CCOs) inside supernova remnants (SNRs) which shows that many of them are placed within local HI minima. The nature of these minima is not clear, but the most likely explanation i
Externí odkaz:
http://arxiv.org/abs/astro-ph/0310694
We have carried out a study of the neutral hydrogen in the direction of the X-ray source 1E 161348-5055, a compact central object (CCO) located in the interior of the supernova remnant (SNR) RCW 103. The HI 21 cm line observations were carried out us
Externí odkaz:
http://arxiv.org/abs/astro-ph/0310100
Publikováno v:
Mon.Not.Roy.Astron.Soc.345:671,2003
We have observed the HI distribution in an area 40' x 40' around the neutron star candidate RX J0822-4300, which is located in the supernova remnant Puppis A. The observations of the 21 cm line were obtained with the Australia Telescope Compact Array
Externí odkaz:
http://arxiv.org/abs/astro-ph/0307065
Using the Australia Telescope Compact Array, we have carried out a survey of the HI emission in the direction of the ``barrel-shaped'' supernova remnant (SNR) G320.4-1.2 (MSH 15-52) and its associated young pulsar B1509-58. The angular resolution of
Externí odkaz:
http://arxiv.org/abs/astro-ph/0110218
Autor:
Dubner, G. M., Giacani, E. B., Goss, W. M., Green, A. J., Nyman, L.-Å., Dubner, G. M., Giacani, E. B., Goss, W. M., Green, A. J., Nyman, L.-Å.
Publikováno v:
Astronomy and Astrophysics; June 2002, Vol. 387 Issue: 3 p1047-1056, 10p
Publikováno v:
Astronomical Journal; Oct1998, Vol. 116 Issue 4, p1842-1855, 14p
Publikováno v:
Astronomical Journal; Aug1998, Vol. 116 Issue 2, p813-822, 10p
Autor:
Reynoso, E. M., Moffett, D. A., Goss, W. M., Dubner, G. M., Dickel, J. R., Reynolds, S. P., Giacani, E. B.
Publikováno v:
Astrophysical Journal; 12/20/1997, Vol. 491 Issue 2, p816-828, 13p