Zobrazeno 1 - 10
of 258
pro vyhledávání: '"Seaquist E"'
Autor:
Wilson, C. D., Warren, B. E., Israel, F. P., Serjeant, S., Attewell, D., Bendo, G. J., Butner, H. M., Chanial, P., Clements, D. L., Golding, J., Heesen, V., Irwin, J., Leech, J., Matthews, H. E., Muhle, S., Mortier, A. M. J., Petitpas, G., Sanchez-Gallego, J. R., Sinukoff, E., Shorten, K., Tan, B. K., Tilanus, R. P. J., Usero, A., Vaccari, M., Wiegert, T., Zhu, M., Alexander, D. M., Alexander, P., Azimlu, M., Barmby, P., Borys, C., Brar, R., Bridge, C., Brinks, E., Brooks, S., Coppin, K., Cote, S., Cote, P., Courteau, S., Davies, J., Eales, S., Fich, M., Hudson, M., Hughes, D. H., Ivison, R. J., Knapen, J. H., Page, M., Parkin, T. J., Pope, A., Rigopoulou, D., Rosolowsky, E., Seaquist, E. R., Spekkens, K., Tanvir, N., van der Hulst, J. M., van der Werf, P., Vlahakis, C., Webb, T. M., Weferling, B., White, G. J.
The James Clerk Maxwell Telescope Nearby Galaxies Legacy Survey (NGLS) comprises an HI-selected sample of 155 galaxies spanning all morphological types with distances less than 25 Mpc. We describe the scientific goals of the survey, the sample select
Externí odkaz:
http://arxiv.org/abs/1206.1629
The question whether or not the initial mass function is universal, i.e. the same in all kinds of environments, is of critical importance for the theory of star formation and still intensely debated. A top-heavy initial mass function may be the resul
Externí odkaz:
http://arxiv.org/abs/1101.1262
There is growing evidence that the properties of the molecular gas in the nuclei of starburst galaxies and in AGN may be very different from those seen in Galactic star forming regions and that a high kinetic temperature in the molecular gas may lead
Externí odkaz:
http://arxiv.org/abs/0901.3468
Using the IRAM 30-m telescope and the 15-m JCMT, we explore the value of para-formaldehyde (p-H_2CO) as a tracer of density and temperature of the molecular gas in external galaxies. The target of our observations are the lobes of the molecular ring
Externí odkaz:
http://arxiv.org/abs/0708.1710
Publikováno v:
Astron.J.134:118-134,2007
We present a comprehensive study of the dust and gas properties in the after-head-on-collision UGC12914/15 galaxy system using multi-transition CO data and SCUBA sub-mm continuum images at both 450 and 850$\mu$m. CO(3-2) line emission was detected in
Externí odkaz:
http://arxiv.org/abs/astro-ph/0703200
Autor:
Seaquist, E. R., Stankovic, M.
Publikováno v:
Astrophys.J.659:347-358,2007
The compact non-thermal sources in M82 and other starburst galaxies are generally thought to be supernova remnants (SNRs). We consider an alternative hypothesis that most are wind driven bubbles (WDBs) associated with very young super star clusters (
Externí odkaz:
http://arxiv.org/abs/astro-ph/0612394
Autor:
Yao, Lihong, Seaquist, E. R.
In this paper, we present an overview of our method of constructing a family of models for the far-infrared, sub-millimeter, and millimeter (FIR/sub-mm/mm) line emission of molecular and atomic gas surrounding massive star formation in starburst gala
Externí odkaz:
http://arxiv.org/abs/astro-ph/0605654
Publikováno v:
Astrophys.J.638:148-156,2006
We present a map of 12CO J=6-5 emission of the nuclear region of the nearby starburst galaxy M82 at resolution 7" taken with the James Clerk Maxwell Telescope (JCMT). This is the highest resolution map yet available at this transition. A detailed qua
Externí odkaz:
http://arxiv.org/abs/astro-ph/0510626
Publikováno v:
Astrophys.J.636:881-890,2006
The effect of a newly born star cluster inside a giant molecular cloud (GMC) is to produce a hot bubble and a thin, dense shell of interstellar gas and dust swept up by the H II expansion, strong stellar winds, and repeated supernova explosions. Lyin
Externí odkaz:
http://arxiv.org/abs/astro-ph/0509554
Publikováno v:
In Journal of Diabetes and Its Complications December 2018 32(12):1097-1099
