Zobrazeno 1 - 10
of 94
pro vyhledávání: '"A. F. Davidsen"'
Publikováno v:
SSRN Electronic Journal.
Publikováno v:
The Astrophysical Journal. 565:773-785
We use a sample of 332 Hubble Space Telescope spectra of 184 QSOs with z > 0.33 to study the typical ultraviolet spectral properties of QSOs, with emphasis on the ionizing continuum. Our sample is nearly twice as large as that of Zheng et al. (1997)
Autor:
Edward M. Murphy, Bruce E. Woodgate, Esther M. Hu, William R. Oegerle, Arthur F. Davidsen, J. B. Hutchings, Kenneth R. Sembach, Lennox L. Cowie
Publikováno v:
The Astrophysical Journal. 560:187-193
We present far-ultraviolet spectroscopy of the cores of the massive cooling flow clusters Abell 1795 and 2597 obtained with FUSE. As the intracluster gas cools through 3x10^5 K, it should emit strongly in the OVI 1032,1038 resonance lines. We report
Autor:
William P. Blair, H. W. Moos, Kenneth R. Sembach, William R. Oegerle, Brad K. Gibson, Edward M. Murphy, George Sonneborn, Edward B. Jenkins, Arthur F. Davidsen, Scott D. Friedman, Blair D. Savage, Jeffrey W. Kruk, Thomas B. Ake, Donald G. York, J. M. Shull, David J. Sahnow
Publikováno v:
The Astrophysical Journal. 538:L31-L34
We have used moderate-resolution (FWHM ≈ 25 km s-1) spectra of active galactic nuclei and QSOs observed by the Far Ultraviolet Spectroscopic Explorer to make the first definitive measurements of absorption by hot gas in high-velocity clouds (HVCs)
Autor:
Bruce E. Woodgate, J. B. Hutchings, Arthur F. Davidsen, Donald G. York, William R. Oegerle, Scott D. Friedman, Richard F. Green, M. S. Brotherton, Kenneth R. Sembach, Gerard A. Kriss, W. Zheng, Mary Elizabeth Kaiser, J. M. Shull
Publikováno v:
The Astrophysical Journal. 538:L17-L21
We present far-ultraviolet spectra of the Seyfert 1 galaxy Mrk 509 obtained in 1999 November with the Far Ultraviolet Spectroscopic Explorer (FUSE). Our data span the observed wavelength range 915-1185 A at a resolution of ~20 km/s. The spectrum show
Publikováno v:
The Astrophysical Journal. 538:395-400
Far-ultraviolet spectra of Venus and Mars in the range 820-1840 A at 4 A resolution were obtained on 13 and 12 March 1995, respectively, by the Hopkins Ultraviolet Telescope (HUT), which was part of the Astro-2 observatory on the Space Shuttle Endeav
Autor:
H. W. Moos, W. C. Cash, L. L. Cowie, A. F. Davidsen, A. K. Dupree, P. D. Feldman, S. D. Friedman, J. C. Green, R. F. Green, C. Gry, J. B. Hutchings, E. B. Jenkins, J. L. Linsky, R. F. Malina, A. G. Michalitsianos, B. D. Savage, J. M. Shull, O. H. W. Siegmund, T. P. Snow, G. Sonneborn, A. Vidal-Madjar, A. J. Willis, B. E. Woodgate, D. G. York, T. B. Ake, B-G Andersson, J. P. Andrews, R. H. Barkhouser, L. Bianchi, W. P. Blair, K. R. Brownsberger, A. N. Cha, P. Chayer, S. J. Conard, A. W. Fullerton, G. A. Gaines, R. Grange, M. A. Gummin, G. Hebrard, G. A. Kriss, J. W. Kruk, D. Mark, D. K. McCarthy, C. L. Morbey, R. Murowinski, E. M. Murphy, W. R. Oegerle, R. G. Ohl, C. Oliveira, S. N. Osterman, D. J. Sahnow, M. Saisse, K. R. Sembach, H. A. Weaver, B. Y. Welsh, E. Wilkinson, W. Zheng
Publikováno v:
The Astrophysical Journal. 538:L1-L6
The Far Ultraviolet Spectroscopic Explorer satellite observes light in the far-ultraviolet spectral region, 905 - 1187 A with high spectral resolution. The instrument consists of four coaligned prime-focus telescopes and Rowland spectrographs with mi
Publikováno v:
The Astrophysical Journal. 482:685-707
We have analyzed the far-ultraviolet (FUV) spectra of six elliptical and S0 galaxies in order to characterize their hot stellar populations. The spectra were obtained using the Hopkins Ultraviolet Telescope (HUT) in March 1995. These data, together w
Autor:
Jay B. Holberg, David S. Finley, Samuel T. Durrance, Gerard A. Kriss, Randy A. Kimble, Jeffrey W. Kruk, R. H. Buss, Arthur F. Davidsen
Publikováno v:
The Astrophysical Journal. 482:546-568
We present the final calibration of the Hopkins Ultraviolet Telescope (HUT) for its flight during the Astro-1 space shuttle mission in 1990 December. The calibration is defined by a comparison between an observation obtained in flight of the hot DA w
Autor:
Arthur F. Davidsen, Hongguang Bi
Publikováno v:
The Astrophysical Journal. 479:523-542
We have performed a detailed statistical study of the evolution of structure in a photoionized intergalactic medium (IGM) using analytical simulations to extend the calculation into the mildly non-linear density regime found to prevail at z = 3. Our