Zobrazeno 1 - 10
of 399
pro vyhledávání: '"Velusamy, T"'
Autor:
Velusamy, T., Adumitroaie, V., Arballo, J., Levin, S. M., Ries, P. A., Dorcey, R., Kreuser-Jenkins, N., Leflang, J., Jauncey, D., Horiuchi, S.
Goldstone Apple Valley Radio Telescope (GAVRT) is a science education partnership among NASA, the Jet Propulsion Laboratory (JPL), and the Lewis Center for Educational Research (LCER), offering unique opportunities for K -12 students and their teache
Externí odkaz:
http://arxiv.org/abs/2007.09184
Goldstone Apple Valley Radio Telescope (GAVRT) is a science education partnership among NASA, the Jet Propulsion Laboratory (JPL), and the Lewis Center for Educational Research (LCER), offering unique opportunities for K -12 students and their teache
Externí odkaz:
http://arxiv.org/abs/2007.05058
Autor:
Langer, W. D., Velusamy, T., Goldsmith, P. F., Pineda, J. L., Chambers, E. T., Sandell, G., Risacher, C., Jacobs, K.
Determining the properties of the warm ionized medium (WIM) at the leading edge of spiral arms is important for understanding its dynamics and cloud formation. The inner edge of the Scutum arm tangency is a unique location in which to disentangle the
Externí odkaz:
http://arxiv.org/abs/1708.02310
The Galactic Central Molecular Zone (CMZ) is a region containing massive and dense molecular clouds, with dynamics driven by a variety of energy sources including a massive black hole. It is thus the nearest template for understanding physical proces
Externí odkaz:
http://arxiv.org/abs/1701.03482
Publikováno v:
Publications of the Astronomical Society of the Pacific, 2020 Sep 01. 132(1015), 1-15.
Externí odkaz:
https://www.jstor.org/stable/26973305
The spiral arm tangencies are ideal lines of sight in which to determine the distribution of interstellar gas components in the spiral arms and study the influence of spiral density waves on the interarm gas in the Milky Way. We present a large scale
Externí odkaz:
http://arxiv.org/abs/1504.03373
Autor:
Langer, W. D., Goldsmith, P. F., Pineda, J. L., Velusamy, T., Requena-Torres, M. A., Wiesemeyer, H.
To determine the properties of the ionized gas at the edge of the CMZ near Sgr E we observed a small portion of the edge of the CMZ near Sgr E with spectrally resolved [C II] 158 micron and [N II] 205 micron fine structure lines at six positions with
Externí odkaz:
http://arxiv.org/abs/1501.06832
Autor:
Sinclair, J.A., Orton, G.S., Fletcher, L.N., Roman, M., de Pater, I., Encrenaz, T., Hammel, H.B., Giles, R.S., Velusamy, T., Moses, J.I., Irwin, P.G.J., Momary, T.W., Rowe-Gurney, N., Tabataba-Vakili, F.
Publikováno v:
In Icarus 15 July 2020 345
Autor:
Velusamy, T., Langer, W. D.
Publikováno v:
A&A 572, A45 (2014)
We determine the source of the diffuse [CII] emission by studying its spatial (radial and vertical) distributions. We used the HIFI [CII] Galactic survey (GOT C+), along with HI, 12CO, and 13CO data toward 354 lines of sight, and several HIFI [CII] a
Externí odkaz:
http://arxiv.org/abs/1409.4788
The distribution of various interstellar gas components and the pressure in the interstellar medium (ISM) is a result of the interplay of different dynamical mechanisms and energy sources on the gas in the Milky Way. The scale heights of the differen
Externí odkaz:
http://arxiv.org/abs/1403.4247