Zobrazeno 1 - 10
of 42
pro vyhledávání: '"O. Vancura"'
Autor:
O. Vancura, Knox S. Long, Jon A. Morse, Patrick Hartigan, John C. Raymond, Richard J. Edgar, William P. Blair, Wilton T. Sanders
Publikováno v:
The Astrophysical Journal. 482:881-890
Ultraviolet emission lines in supernova remnants (SNRs) provide important clues to the shock velocities, densities, grain destruction, and thermal structure of the cooling regions in these objects. However, several of the brightest ultraviolet emissi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::68195b7b75ebab19c4b53db0c12d1493
https://doi.org/10.1086/304183
https://doi.org/10.1086/304183
Autor:
Gerard A. Kriss, Arthur F. Davidsen, O. Vancura, Samuel T. Durrance, W. V. Dixon, C. W. Bowers, Knox S. Long, Paul D. Feldman, R. A. Kimble, Richard C. Henry, Henry C. Ferguson, Jeffrey W. Kruk, William P. Blair, H. W. Moos
Publikováno v:
Nature. 351:128-130
Sciama's hypothesis that the dark matter associated with galaxies, galaxy clusters, and the intergalactic medium consists of tau neutrinos of rest mass 28-30 eV whose decay generates ultraviolet photons of energy roughly 14-15 eV, has been tested usi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5bd22b1eb20c4892650efa5428ebb513
https://doi.org/10.1038/351128a0
https://doi.org/10.1038/351128a0
Publikováno v:
AIP Conference Proceedings.
We have searched the Einstein HRI images of the supernova remnant N49 for evidence of any point‐like x‐ray enhancement within the error box of the repeating gamma ray burst source GBS 0525‐66, the source of the 5 March 1979 and other bursts. Al
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4eed28c545886c0bc48df85ecb51638d
https://doi.org/10.1063/1.44225
https://doi.org/10.1063/1.44225
Publikováno v:
Scopus-Elsevier
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5cae7b3b677b9f1f2d43edf4cbb2a3fc
https://doi.org/10.1086/177467
https://doi.org/10.1086/177467
Publikováno v:
The Astrophysical Journal. 457:244
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::45b81267e67b49152ab2f87ee356f7b7
https://doi.org/10.1086/176725
https://doi.org/10.1086/176725
Publikováno v:
The Astronomical Journal. 110:312
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2543f8ba9fecaee5e4bd01f2245a5892
https://doi.org/10.1086/117521
https://doi.org/10.1086/117521
Publikováno v:
Scopus-Elsevier
We present an X-ray study of the Tycho supernova remnant utilizing archival data from the high-resolution imagers (HRIs) on Einstein and ROSAT, the low-energy imaging telescopes (LEITs) on EXOSAT, and spectral data from the Broad Band X-ray Telescope
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ca38a54f12da25185ff9180f1c385ebb
https://doi.org/10.1086/175391
https://doi.org/10.1086/175391
Publikováno v:
The Astrophysical Journal. 431:188
We have constructed models that predict the dynamic evolution and infrared (IR) emission of grains behind nonradiative shock waves. We present a self-consistent treatment of the effect of grain destruction and heating on the ionization structure and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1e0c3f3c8b7c41677f81515bb58c7803
https://doi.org/10.1086/174477
https://doi.org/10.1086/174477
Publikováno v:
The Astrophysical Journal. 417:663
We have used the Voyager 1 and 2 Ultraviolet Spectrometers to study the far-ultraviolet emissions from different types of shock waves in the Cygnus Loop. In the southeast and northern parts of the supernova remnant (SNR), we have measured the O(VI) l
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::26c7f6f5a0f1831ab15ff9d76c31440c
https://doi.org/10.1086/173344
https://doi.org/10.1086/173344
Autor:
Richard C. Henry, W. Van Dyke Dixon, Knox S. Long, H. Warren Moos, Jeffrey W. Kruk, Randy A. Kimble, Gerard A. Kriss, Samuel T. Durrance, Paul D. Feldman, Charles W. Bowers, O. Vancura, William P. Blair, Henry C. Ferguson, Arthur F. Davidsen
Publikováno v:
The Astrophysical Journal. 404:663
During the Astro-l mission in 1990 December, the Hopkins Ultraviolet Telescope (HUT) was used to observe the extreme ultraviolet spectrum (415-912 A) of the hot DA white dwarf GI91-B2B. Absorption by neutral helium shortward of the 504 A He I absorpt
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8a8db7ed12510c7117478c6061944974
https://doi.org/10.1086/172319
https://doi.org/10.1086/172319