Zobrazeno 1 - 10
of 92
pro vyhledávání: '"Oegerle, W."'
Autor:
Postman, M., Traub, W., Krist, J., Stapelfeldt, K., Brown, R., Oegerle, W., Lo, A., Clampin, M., Soummer, R., Wiseman, J., Mountain, M.
The Advanced Technology Large Aperture Space Telescope (ATLAST) is a set of mission concepts for the next generation UV-Optical-Near Infrared space telescope with an aperture size of 8 to 16 meters. ATLAST, using an internal coronagraph or an externa
Externí odkaz:
http://arxiv.org/abs/0911.3841
Autor:
Bowen, D. V., Jenkins, E. B., Tripp, T. M., Sembach, K. R., Savage, B. D., Moos, H. W., Oegerle, W. R., Friedman, S. D., Gry, C., Kruk, J. W., Murphy, E., Sankrit, R., Shull, J. M., Sonneborn, G., York, D. G.
Publikováno v:
Astrophys.J.Suppl.176:59-163,2008
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
Externí odkaz:
http://arxiv.org/abs/0711.0005
Publikováno v:
Astrophys.J.622:377-389,2005
We report the results of a survey of OVI 1032 absorption along the lines of sight to 25 white dwarfs in the local interstellar medium (LISM) obtained with the Far Ultraviolet Spectroscopic Explorer (FUSE). We find that interstellar OVI absorption alo
Externí odkaz:
http://arxiv.org/abs/astro-ph/0411065
We have used the Far Ultraviolet Spectroscopic Explorer to search for OVI 1031.926, 1037.617 A emission in the halos of the edge-on spiral galaxies NGC4631 and NGC891. In NGC4631, we detected OVI in emission toward a soft X-ray bubble above a region
Externí odkaz:
http://arxiv.org/abs/astro-ph/0304079
Autor:
Wakker, B. P., Savage, B. D., Sembach, K. R., Richter, P., Meade, M., Jenkins, E. B., Shull, J. M., Ake, T. B., Blair, W. P., Friedman, S. D., Green, J. C., Green, R. F., Kruk, J. W., Moos, H. W., Murphy, E. M., Oegerle, W. R., Sahnow, D. J., Sonneborn, G., Wilkinson, E., York, D. G.
We present FUSE observations of OVI absorption in a sample of 100 extragalactic targets and 2 distant halo stars. We describe the details of the calibration, alignment in velocity, continuum fitting, and manner in which contaminants were removed (Gal
Externí odkaz:
http://arxiv.org/abs/astro-ph/0208009
Autor:
Kruk, J. W., Howk, J. C., Andre, M., Moos, H. W., Oegerle, W. R., Oliveira, C., Sembach, K. R., Chayer, P., Linsky, J. L., Wood, B. E., Ferlet, R., Hebrard, G., Lemoine, M., Vidal-Madjar, A., Sonneborn, G.
Publikováno v:
Astrophys.J.Suppl. 140 (2002) 19-36
We present an analysis of interstellar absorption along the line of sight to the nearby white dwarf star HZ43A. The distance to this star is 68+/-13 pc, and the line of sight extends toward the north Galactic pole. Column densities of OI, NI, and NII
Externí odkaz:
http://arxiv.org/abs/astro-ph/0201298
Autor:
Sonneborn, G., Andre, M., Oliveira, C., Hebrard, G., Howk, J. C., Tripp, T. M., Chayer, P., Friedman, S. D., Kruk, J. W., Jenkins, E. B., Lemoine, M., Moos, H. W., Oegerle, W. R., Sembach, K. R., Vidal-Madjar, A.
Publikováno v:
Astrophys.J.Suppl.140:51-66,2002
High resolution far-ultraviolet spectra of the O-type subdwarf BD +28 4211 were obtained with the Far Ultraviolet Spectroscopic Explorer (FUSE) to measure the interstellar deuterium, nitrogen, and oxygen abundances in this direction. The interstellar
Externí odkaz:
http://arxiv.org/abs/astro-ph/0201177
Autor:
Moos, H. W., Sembach, K. R., Vidal-Madjar, A., York, D. G., Friedman, S. D., Hebrard, G., Kruk, J. W., Lehner, N., Lemoine, M., Sonneborn, G., Wood, B. E., Ake, T. B., Andre, M., Blair, W. P., Chayer, P., Gry, C., Dupree, A. K., Ferlet, R., Feldman, P. D., Green, J. C., Howk, J. C., Hutchings, J. B., Jenkins, E. B., Linsky, J. L., Murphy, E. M., Oegerle, W. R., Oliveira, C., Roth, K., Sahnow, D. J., Savage, B. D., Shull, J. M., Tripp, T. M., Weiler, E. J., Welsh, B. Y., Wilkinson, E., Woodgate, B. E.
Publikováno v:
Astrophys.J.Suppl.140:3-18,2002
Observations obtained with the Far Ultraviolet Spectroscopic Explorer (FUSE) have been used to determine the column densities of D I, O I, and N I along seven sight lines that probe the local interstellar medium (LISM) at distances from 37 pc to 179
Externí odkaz:
http://arxiv.org/abs/astro-ph/0112519
Autor:
Lemoine, M., Vidal-Madjar, A., Hebrard, G., Desert, J. -M., Ferlet, R., Etangs, A. Lecavelier des, Howk, J. C., Andre, M., Blair, W. P., Friedman, S. D., Kruk, J. W., Lacour, S., Moos, H. W., Sembach, K., Chayer, P., Jenkins, E. B., Koester, D., Linsky, J. L., Wood, B. E., Oegerle, W. R., Sonneborn, G., York, D. G.
High-resolution spectra of the hot white dwarf G191-B2B, covering the wavelength region 905-1187A, were obtained with the Far Ultraviolet Spectroscopic Explorer (FUSE). This data was used in conjunction with existing high-resolution Hubble Space Tele
Externí odkaz:
http://arxiv.org/abs/astro-ph/0112180
Autor:
Hebrard, G., Lemoine, M., Vidal-Madjar, A., Desert, J. -M., Etangs, A. Lecavelier des, Ferlet, R., Wood, B. E., Linsky, J. L., Kruk, J. W., Chayer, P., Lacour, S., Blair, W. P., Friedman, S. D., Moos, H. W., Sembach, K. R., Sonneborn, G., Oegerle, W. R., Jenkins, E. B.
We present a deuterium abundance analysis of the line of sight toward the white dwarf WD2211-495 observed with the Far Ultraviolet Spectroscopic Explorer (FUSE). Numerous interstellar lines are detected on the continuum of the stellar spectrum. A tho
Externí odkaz:
http://arxiv.org/abs/astro-ph/0112181