Zobrazeno 1 - 10
of 39
pro vyhledávání: '"K. R. Sembach"'
Publikováno v:
Vol. 53, Issue 2. 53
Autor:
R. J. Weymann, Edward B. Jenkins, Robert F. Carswell, Gerard M. Williger, K. R. Sembach, Todd M. Tripp, L. Haberzettl, Romeel Davé, Sara R. Heap
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 405:1736-1758
We present an analysis of the Ly-a forest toward 3C 273 from the Space Telescope Imaging Spectrograph at ~7 km/s resolution, along with re-processed data from the Far Ultraviolet Spectroscopic Explorer. The high UV flux of 3C 273 allows us to probe t
Autor:
J. P. Grimes, Alessandra Aloisi, Claus Leitherer, K. R. Sembach, Crystal L. Martin, Daniela Calzetti, Gerhardt R. Meurer, D. K. Strickland, Timothy M. Heckman
Publikováno v:
The Astrophysical Journal Supplement Series. 181:272-320
We have analyzed FUSE (905-1187 A) spectra of a sample of 16 local starburst galaxies. These galaxies cover almost three orders of magnitude in star-formation rates and over two orders of magnitude in stellar mass. Absorption features from the stars
Autor:
Eric J. Murphy, Cecile Gry, D. G. York, Scott D. Friedman, David V. Bowen, Edward B. Jenkins, Blair D. Savage, William R. Oegerle, R. Sankrit, George Sonneborn, Jeffrey W. Kruk, H. W. Moos, Todd M. Tripp, J. M. Shull, K. R. Sembach
Publikováno v:
The Astrophysical Journal Supplement Series. 176:59-163
To probe the distribution and physical characteristics of interstellar gas at temperatures T ~ 3e5 K in the disk of the Milky Way, we have used the Far Ultraviolet Spectroscopic Explorer (FUSE) to observe absorption lines of OVI toward 148 early-type
Autor:
J. P. Grimes, William V. Dixon, A. F. Ptak, Timothy M. Heckman, C. G. Hoopes, D. K. Strickland, K. R. Sembach, Alessandra Aloisi, Roderik Overzier
Publikováno v:
The Astrophysical Journal. 668:891-905
We have re-analyzed FUSE data and obtained new Chandra observations of Haro 11, a local (D_L=88 Mpc) UV luminous galaxy. Haro 11 has a similar far-UV luminosity (10^10.3 L_\odot), UV surface brightness (10^9.4 L_\odot kpc^-2), SFR, and metallicity to
Publikováno v:
Astronomy & Astrophysics. 445:827-842
We discuss physical properties and baryonic content of broad Ly alpha absorbers (BLAs) at low redshift. These absorption systems, recently discovered in high-resolution, high-signal to noise quasar absorption line spectra, possibly trace the warm-hot
Publikováno v:
Proceedings of the International Astronomical Union. 1:162-167
Publikováno v:
The Astrophysical Journal. 619:863-883
High-quality Far-Ultraviolet Spectroscopic Explorer (FUSE) observations at 20 km /s resolution of interstellar and intergalactic absorption from 910 to 1187 A are presented for the X-ray bright BL Lac object Mrk 421. In this study we consider the O V
Autor:
K. R. Sembach
Publikováno v:
Symposium - International Astronomical Union. 216:274-289
There is increasing observational evidence that hot, highly-ionized interstellar and intergalactic gas plays a significant role in the evolution of galaxies in the local universe. Recent observations from several ultraviolet and X-ray observatories h
Publikováno v:
Symposium - International Astronomical Union. 217:147-153
We summarize the results of the Far-Ultraviolet Spectroscopic Explorer (FUSE) program to study O VI in the Milky Way halo. Spectra of 100 extragalactic objects and two distant halo stars are analyzed to obtain measures of O VI absorption along paths