Zobrazeno 1 - 10
of 189
pro vyhledávání: '"B. Aschenbach"'
Publikováno v:
The Astrophysical Journal. 568:L49-L52
We present a {\it Chandra} ACIS observation of SNR G54.1+0.3. This supernova remnant is resolved into several distinct X-ray emitting components: a central bright point-like source (CXOU J193030.13+185214.1), a surrounding ring, bipolar elongations,
Autor:
B. Aschenbach
Publikováno v:
Nuclear Physics B - Proceedings Supplements. 69:78-87
A summary of X-ray observations of supernova remnants is presented including the explosion fragment A of the Vela SNR, Tycho, N132D, RX J0852-4622, the Crab Nebula and the 'bulls eye', and SN 1987A, high-lighting the progress made with Chandra and XM
Autor:
D.H. Hartmann, P. Predehl, J. Greiner, R. Egger, J. Trümper, B. Aschenbach, A.F. Iyudin, R.D. Diehl, U. Oberlack, V. Schönfelder, M.D. Leising, L.-S. The, F.X. Timmes, S.E. Woosley, R. Hoffman, N. Langer, G. Garcia-Segura
Publikováno v:
Nuclear Physics A. 621:83-91
The Galactic supernova remnant Cas A is believed to be the result of a recent (∼ 300 yrs) and nearby (D ∼ 3 kpc) explosion of a massive star. The discovery of gamma-ray line emission due to radioactive 44 Ti with COMPTEL supports the massive star
Autor:
R. A. Harrison, E. C. Sawyer, M. K. Carter, A. M. Cruise, R. M. Cutler, A. Fludra, R. W. Hayes, B. J. Kent, J. Lang, D. J. Parker, J. Payne, C. D. Pike, S. C. Peskett, A. G. Richards, J. L. Gulhane, K. Norman, A. A. Breeveld, E. R. Breeveld, K. F. Al Janabi, A. J. Mccalden, J. H. Parkinson, D. G. Self, P. D. Thomas, A. I. Poland, R. J. Thomas, W. T. Thompson, O. Kjeldseth-Moe, P. Brekke, J. Karud, P. Maltby, B. Aschenbach, H. Bräuninger, M. Kühne, J. Hollandt, O. H. W. Siegmund, M. C. E. Huber, A. H. Gabriel, H. E. Mason, B. J. I. Bromage
Publikováno v:
Solar Physics. 162:233-290
We report the results of our XMM-Newton monitoring of SN 1987A. The ongoing propagation of the supernova blast wave through the inner circumstellar ring caused a drastic increase in X-ray luminosity during the last years, enabling detailed high resol
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b7a168877c6851872d9128047137ec73
Autor:
B. Aschenbach
Publikováno v:
Highlights of Astronomy. 9:223-228
Spectrally resolved X-ray images of the Cygnus Loop and the Vela supernova remnant have been obtained during the ROSAT all sky survey. The remnants show highly filamentary brightness distributions. Temperatures between 1·106 K and 10·106 K have bee
Autor:
A. Wells, D.H. Lumb, K.A. Pounds, G.C. Stewart, B. Aschenbach, H. Brauninger, G. Hasinger, J. Trumper, O. Citterio, L. Scarsi, A. Peacock, B. Taylor
Publikováno v:
International Astronomical Union Colloquium. 115:318-330
The Joint European X-Ray Telescope, JET-X, is one of the core instruments of the scientific payload of the USSR SPECTRUM-X astrophysics mission due for launch in 1993. The JET-X instrument concept is described and its scientific performance and capab
Publikováno v:
ESO Astrophysics Symposia ISBN: 9783540747123
Relativistic Astrophysics Legacy and Cosmology – Einstein’s
Relativistic Astrophysics Legacy and Cosmology – Einstein’s
"Relativistic Astrophysics and Cosmology" have developed into important and fruitful research areas with a hitherto unprecented public interest. The year 2005, which marked the 100th anniversary of the 'annus mirabilis', that year in which Albert Ein
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1ade422c0c70a78429b3663046f123d7
https://doi.org/10.1007/978-3-540-74713-0
https://doi.org/10.1007/978-3-540-74713-0
Publikováno v:
The Astrophysical Journal. 805:142
Thermal X-ray emission from young supernova remnants (SNRs) is usually dominated by the emission lines of the supernova (SN) ejecta, which are widely believed being crossed and thus heated by the inwards propagating reverse shock (RS). Previous works
Autor:
B. Aschenbach
Publikováno v:
Growing Black Holes: Accretion in a Cosmological Context ISBN: 3540252754
For very fast spinning black holes with a>0.9953 the orbital velocity of a test particle unexpectly shows a positive radial gradient for low orbits, an effect of GR which has been overlooked so far. For a=0.99616 the maximum radial change of the orbi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e0ec1acb14234941fa75b6e9783b49e0
https://doi.org/10.1007/11403913_54
https://doi.org/10.1007/11403913_54