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pro vyhledávání: '"Hoopes C"'
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Autor:
Beirão, P., Armus, L., Lehnert, M. D., Guillard, P., Heckman, T., Draine, B., Hollenbach, D., Walter, F., Sheth, K., Smith, J. D., Shopbell, P., Boulanger, F., Surace, J., Hoopes, C., Engelbracht, C.
We have mapped the superwind/halo region of the nearby starburst galaxy M82 in the mid-infrared with $Spitzer-IRS$. The spectral regions covered include the H$_2 S(1)-S(3)$, [NeII], [NeIII] emission lines and PAH features. We estimate the total warm
Externí odkaz:
http://arxiv.org/abs/1505.04069
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
Autor:
Grimes, J. P., Heckman, T., Strickland, D., Dixon, W. V., Sembach, K., Overzier, R., Hoopes, C., Aloisi, A., Ptak, A.
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
Externí odkaz:
http://arxiv.org/abs/0707.0693
Autor:
Wong, O. I., Meurer, G. R., Bekki, K., Hanish, D. J., Kennicutt, R. C., Bland-Hawthorn, J., Ryan-Weber, E. V., Koribalski, B., Kilborn, V. A., Putman, M. E., Heiner, J. S., Webster, R. L., Allen, R. J., Dopita, M. A., Doyle, M. T., Drinkwater, M. J., Ferguson, H. C., Freeman, K. C., Heckman, T. M., Hoopes, C., Knezek, P. M., Meyer, M. J., Oey, M. S., Seibert, M., Smith, R. C., Staveley-Smith, L., Thilker, D., Werk, J., Zwaan, M. A.
Publikováno v:
Mon.Not.Roy.Astron.Soc.370:1607-1611,2006
We have found the peculiar galaxy NGC922 to be a new drop-through ring galaxy using multi-wavelength (UV-radio) imaging and spectroscopic observations. Its `C'-shaped morphology and tidal plume indicate a recent strong interaction with its companion
Externí odkaz:
http://arxiv.org/abs/astro-ph/0605613
Publikováno v:
Astrophys.J.648:310-322,2006
We have analyzed FUSE, XMM, and Chandra observations of VV 114, a local galaxy merger with strong similarities to typical high-redshift Lyman Break Galaxies (LBGs). Diffuse thermal X-ray emission encompassing VV114 has been observed by Chandra and XM
Externí odkaz:
http://arxiv.org/abs/astro-ph/0605241
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:
Bianchi, Luciana, Thilker, D., Burgarella, D., Friedman, P., Hoopes, C., Boissier, S., de Paz, A. Gil, Barlow, T., Byun, Y. -I., Donas, J., Forster, K., Heckman, T., Jelinsky, P., Lee, Y-W, Madore, B., Malina, R., Martin, C., Milliard, B., Morrissey, P., Neff, S., Rich, M., Schiminovich, D., Siegmund, O., Small, T., Szalay, A., Welsh, B., Wyder, T.
Publikováno v:
Astrophys.J. 619 (2005) L71-L74
The GALEX (Galaxy Evolution Explorer) Nearby Galaxies Survey is providing deep far-UV and near-UV imaging for a representative sample of galaxies in the local universe. We present early results for M51 and M101, from GALEX UV imaging and SDSS optical
Externí odkaz:
http://arxiv.org/abs/astro-ph/0411408
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