Zobrazeno 1 - 10
of 39
pro vyhledávání: '"Gomez, E. L."'
Autor:
Forgan, D. H., Rowlands, K., Gomez, H. L., Gomez, E. L., Schofield, S. P., Dunne, L., Maddox, S.
The process of planet formation offers a rich source of dust production via grain growth in protostellar discs, and via grinding of larger bodies in debris disc systems. Chemical evolution models, designed to follow the build up of metals and dust in
Externí odkaz:
http://arxiv.org/abs/1708.07053
Autor:
De Vis, P., Gomez, H. L., Schofield, S. P., Maddox, S., Dunne, L., Baes, M., Cigan, P., Clark, C. J. R., Gomez, E. L., Lara-López, M., Owers, M.
We combine samples of nearby galaxies with Herschel photometry selected on their dust, metal, HI, and stellar mass content, and compare these to chemical evolution models in order to discriminate between different dust sources. In a companion paper,
Externí odkaz:
http://arxiv.org/abs/1705.02340
Autor:
Brown, T. M., Baliber, N., Bianco, F. B., Bowman, M., Burleson, B., Conway, P., Crellin, M., Depagne, É., De Vera, J., Dilday, B., Dragomir, D., Dubberley, M., Eastman, J. D., Elphick, M., Falarski, M., Foale, S., Ford, M., Fulton, B. J., Garza, J., Gomez, E. L., Graham, M., Greene, R., Haldeman, B., Hawkins, E., Haworth, B., Haynes, R., Hidas, M., Hjelstrom, A. E., Howell, D. A., Hygelund, J., Lister, T. A., Lobdill, R., Martinez, J., Mullins, D. S., Norbury, M., Parrent, J., Paulson, R., Petry, D. L., Pickles, A., Posner, V., Rosing, W. E., Ross, R., Sand, D. J., Saunders, E. S., Shobbrook, J., Shporer, A., Street, R. A., Thomas, D., Tsapras, Y., Tufts, J. R., Valenti, S., Horst, K. Vander, Walker, Z., White, G., Willis, M.
Las Cumbres Observatory Global Telescope (LCOGT) is a young organization dedicated to time-domain observations at optical and (potentially) near-IR wavelengths. To this end, LCOGT is constructing a world-wide network of telescopes, including the two
Externí odkaz:
http://arxiv.org/abs/1305.2437
Autor:
Gomez, H. L., Krause, O., Barlow, M. J., Swinyard, B. M., Owen, P. J., Clark, C. J. R., Matsuura, M., Gomez, E. L., Rho, J., Besel, M. -A., Bouwman, J., Gear, W. K., Henning, Th., Ivison, R. J., Polehampton, E. T., Sibthorpe, B.
Whether supernovae are major sources of dust in galaxies is a long-standing debate. We present infrared and submillimeter photometry and spectroscopy from the Herschel Space Observatory of the Crab Nebula between 51 and 670 micron as part of the Mass
Externí odkaz:
http://arxiv.org/abs/1209.5677
Autor:
Gomez, H. L., Clark, C. J. R., Nozawa, T., Krause, O., Gomez, E. L., Matsuura, M., Barlow, M. J., Besel, M. -A., Dunne, L., Gear, W. K., Hargrave, P., Henning, Th., Ivison, R. J., Sibthorpe, B., Swinyard, B. M., Wesson, R.
The origin of interstellar dust in galaxies is poorly understood, particularly the relative contributions from supernovae and the cool stellar winds of low-intermediate mass stars. Here, we present Herschel PACS and SPIRE photometry at 70-500um of th
Externí odkaz:
http://arxiv.org/abs/1111.6627
Autor:
Gomez, H. L., Vlahakis, C., Stretch, C. M., Dunne, L., Eales, S. A., Beelen, A., Gomez, E. L., Edmunds, M. G.
Previous submillimetre (submm) observations detected 0.7 solar masses of cool dust emission around the Luminous Blue Variable (LBV) star Eta Carinae. These observations were hindered by the low declination of Eta Carinae and contamination from free-f
Externí odkaz:
http://arxiv.org/abs/0911.0176
Publikováno v:
".Astronomy: Networked Astronomy and the New Media", 2009, edited by R.J. Simpson, D. Ward-Thompson
We present a brief introduction to the phenomenon of "social networking" and its potentially powerful use as an astronomy outreach and educational tool. We briefly discuss the development of applications for websites and facebook and the use of web t
Externí odkaz:
http://arxiv.org/abs/0903.0266
Autor:
Gomez, E. L., Williams, R. J. R.
Publikováno v:
Mon.Not.Roy.Astron.Soc. 344 (2003) 725
In this paper, we study the structure and stability of line driven winds using numerical hydrodynamic simulations. We calculate the radiation force from an explicit non-local solution of the radiation transfer equation, rather than a Sobolev approxim
Externí odkaz:
http://arxiv.org/abs/astro-ph/0305598
Autor:
Gomez, E. L., Fitzgerald, M. T.
Publikováno v:
Astronomical Review; January 2017, Vol. 13 Issue: 1 p28-68, 41p
Akademický článek
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