Zobrazeno 1 - 10
of 28
pro vyhledávání: '"Hoopes, C. G."'
Autor:
Meurer, Gerhardt R., Wong, O. I., Kim, J. H., Hanish, D. J., Heckman, T. M., Werk, J., Bland-Hawthorn, J., Dopita, M. A., Zwaan, M. A., Koribalski, B., Seibert, M., Thilker, D. A., Ferguson, H. C., Webster, R. L., Putman, M. E., Knezek, P. M., Doyle, M. T., Drinkwater, M. J., Hoopes, C. G., Kilborn, V. A., Meyer, M., Ryan-Weber, E. V., Smith, R. C., Staveley-Smith, L.
Publikováno v:
Astrophys.J.695:765-780,2009
Many results in modern astrophysics rest on the notion that the Initial Mass Function (IMF) is universal. Our observations of HI selected galaxies in the light of H-alpha and the far-ultraviolet (FUV) challenge this notion. The flux ratio H-alpha/FUV
Externí odkaz:
http://arxiv.org/abs/0902.0384
Publikováno v:
Mon.Not.Roy.Astron.Soc.362:626-648,2005
In this paper we present high-resolution hydrodynamical models of warm ionized clouds embedded in a superwind, and compare the OVI and soft X-ray properties to the existing observational data. These models include thermal conduction, which we show pl
Externí odkaz:
http://arxiv.org/abs/astro-ph/0506645
Thanks to their proximity, local starbursts are perfectly suited for high-resolution and sensitivity multiwavelength observations aimed to test our ideas about star formation, evolution of massive stars, physics and chemical evolution of the interste
Externí odkaz:
http://arxiv.org/abs/astro-ph/0411609
Autor:
Thilker, D. A., Hoopes, C. G., Bianchi, L., Boissier, S., Rich, M., Seibert, M., Friedman, P. G., Rey, S., Buat, V., Barlow, T. A., Byun, Y., Donas, J., Forster, K., Heckman, T. M., Jelinsky, P. N., Lee, Y., Madore, B. F., Malina, R. F., Martin, C., Milliard, B., Morrissey, P. F., Neff, S. G., Schiminovich, D., Siegmund, O. H. W., Small, T., Szalay, A. S., Welsh, B. Y., Wyder, T. K.
Publikováno v:
Astrophys.J. 619 (2005) L67-L70
We present Galaxy Evolution Explorer (GALEX) far-UV and near-UV mosaic observations covering the entirety of M31 and M33. For both targets, we measure the decline of surface brightness (in FUV and NUV) and changes in FUV--NUV color as a function of g
Externí odkaz:
http://arxiv.org/abs/astro-ph/0411311
Autor:
Hoopes, C. G., Heckman, T. M., Strickland, D. K., Seibert, M., Madore, B. F., Rich, R. M., Bianchi, L., de Paz, A. Gil, Burgarella, D., Thilker, D. A., Friedman, P. G., Barlow, T. A., Byun, Y. -I., Donas, J., Forster, K., Jelinsky, P. N., Lee, Y. -W., Malina, R. F., Martin, D. C., Milliard, B., Morrissey, P. F., Neff, S. G., Schiminovich, D., Siegmund, O. H. W., Small, T., Szalay, A. S., Welsh, B. Y., Wyder, T. K.
Publikováno v:
Astrophys.J. 619 (2005) L99-L102
We present Galaxy Evolution Explorer (GALEX) images of the prototypical edge-on starburst galaxies M82 and NGC253. Our initial analysis is restricted to the complex of ultraviolet (UV) filaments in the starburst-driven outflows in the galaxy halos. T
Externí odkaz:
http://arxiv.org/abs/astro-ph/0411309
The determination of the metal abundances in the neutral interstellar medium of dwarf star-forming galaxies is a key step in understanding their physical and chemical evolution. This type of investigation has been possible in the last 5 years thanks
Externí odkaz:
http://arxiv.org/abs/astro-ph/0410072
Autor:
Hoopes, C. G., Sembach, K. R., Heckman, T. M., Meurer, G. R., Aloisi, A., Calzetti, D., Leitherer, C., Martin, C. L.
Publikováno v:
Astrophys.J. 612 (2004) 825-836
(Abridged) We have used the Far Ultraviolet Spectroscopic Explorer (FUSE) to search for H_2 absorption in five starburst galaxies: NGC 1705, NGC 3310, NGC 4214, M83 (NGC 5236), and NGC 5253. We tentatively detect weak absorption by H_2 in M83 and NGC
Externí odkaz:
http://arxiv.org/abs/astro-ph/0406378
Publikováno v:
Astrophys.J.606:829-852,2004
We investigate how the empirical properties of hot X-ray-emitting gas in a sample of seven starburst and three normal edge-on spiral galaxies (a sample which covers the full range of star-formation intensity found in disk galaxies) correlate with the
Externí odkaz:
http://arxiv.org/abs/astro-ph/0306598
We present arcsecond resolution Chandra X-ray and ground-based optical H-alpha imaging of a sample of ten edge-on star-forming disk galaxies (seven starburst and three ``normal'' spiral galaxies), a sample which covers the full range of star-formatio
Externí odkaz:
http://arxiv.org/abs/astro-ph/0306592
Publikováno v:
Astrophys.J. 595 (2003) 760-778
We report on new FUSE far-UV spectroscopy of the most metal-poor blue compact dwarf galaxy I Zw 18. The new data represent an improvement over previous FUSE spectra by a factor of 1.7 in the signal-to-noise. Together with a larger spectral coverage (
Externí odkaz:
http://arxiv.org/abs/astro-ph/0306290