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pro vyhledávání: '"Vutisalchavakul, Nalin"'
Autor:
Vutisalchavakul, Nalin
There has been many recent observations in the area of star formation. High-resolution observations of other galaxies enabled a study of extragalactic star formation in more detailed while large scale surveys of the Milky Way enabled a more comprehen
Externí odkaz:
http://hdl.handle.net/2152/31368
The relations between star formation and properties of molecular clouds are studied based on a sample of star forming regions in the Galactic Plane. Sources were selected by having radio recombination lines to provide identification of associated mol
Externí odkaz:
http://arxiv.org/abs/1607.06518
We examined the relations between molecular gas surface density and star formation rate surface density in a 11 square degree region of the Galactic Plane. Dust continuum at 1.1 mm from the Bolocam Galactic Plane Survey and 22 micron emission from th
Externí odkaz:
http://arxiv.org/abs/1409.5468
We test some ideas for star formation relations against data on local molecular clouds. On a cloud by cloud basis, the relation between the surface density of star formation rate and surface density of gas divided by a free-fall time, calculated from
Externí odkaz:
http://arxiv.org/abs/1401.3287
Autor:
Blanc, Guillermo A., Weinzirl, Tim, Song, Mimi, Heiderman, Amanda, Gebhardt, Karl, Jogee, Shardha, Evans II, Neal J., Bosch, Remco C. E. van den, Luo, Rongxin, Drory, Niv, Fabricius, Maximilian, Fisher, David, Hao, Lei, Kaplan, Kyle, Marinova, Irina, Vutisalchavakul, Nalin, Yoachim, Peter
We present the survey design, data reduction, and spectral fitting pipeline for the VIRUS-P Exploration of Nearby Galaxies (VENGA). VENGA is an integral field spectroscopic survey, which maps the disks of 30 nearby spiral galaxies. Targets span a wid
Externí odkaz:
http://arxiv.org/abs/1303.1552
We have tested some relations for star formation rates used in extra-galactic studies for regions within the Galaxy. In nearby molecular clouds, where the IMF is not fully-sampled, the dust emission at 24 micron greatly underestimates star formation
Externí odkaz:
http://arxiv.org/abs/1302.1858
We present the results of a study of differential rotation on the K2 IV primary of the RS CVn binary II Pegasi (HD 224085) performed by inverting light curves to produce images of the dark starspots on its surface. The data were obtained in the stand
Externí odkaz:
http://arxiv.org/abs/1009.2308
Akademický článek
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Publikováno v:
Astrophysical Journal; 02/20/2014, Vol. 782 Issue 2, p114-126, 13p
Publikováno v:
Astrophysical Journal; 3/10/2013, Vol. 765 Issue 2, p1-13, 13p