Zobrazeno 1 - 10
of 47
pro vyhledávání: '"R. L. Snell"'
Autor:
Itziar Aretxaga, Omaira González-Martín, Martín Herrera-Endoqui, R. L. Snell, Gopal Narayanan, C. A. Negrete, M. S. Yun, M. Martínez-Paredes, A. Caldú-Primo, Irene Cruz-González, V. H. Chavushyan, Erika Benítez, Giovanni G. Fazio, Elena Jiménez-Bailón, David Hiriart, David H. Hughes, Arturo I. Gómez-Ruiz, J. Jesús González, Yair Krongold, J. M. Rodríguez-Espinosa
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 499:2042-2050
As part of the Early Science Large Millimeter Telescope projects, we report the detection of nine double-peaked molecular lines, produced by a rotating molecular torus, in the ultraluminous infrared galaxies (ULIRG) – Compton-thick active galactic
Autor:
Edith Falgarone, U. A. Yildiz, Jorge L. Pineda, R. L. Snell, Paul F. Goldsmith, Mark H. Heyer
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 461 (4), pp.3918-3926. ⟨10.1093/mnras/stw1567⟩
Monthly Notices of the Royal Astronomical Society, 2016, 461 (4), pp.3918-3926. ⟨10.1093/mnras/stw1567⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 461 (4), pp.3918-3926. ⟨10.1093/mnras/stw1567⟩
Monthly Notices of the Royal Astronomical Society, 2016, 461 (4), pp.3918-3926. ⟨10.1093/mnras/stw1567⟩
The origin of striations aligned along the local magnetic field direction in the translucent envelope of the Taurus molecular cloud is examined with new observations of 12CO and 13CO J=2-1 emission obtained with the 10~m submillimeter telescope of th
Autor:
A. Montaña, Roberto Terlevich, Olga Vega, Min S. Yun, David H. Hughes, Itziar Aretxaga, V. De la Luz, Kamal Souccar, Kimberly S. Scott, R. L. Snell, F. P. Schloerb, Grant W. Wilson, David J. Wilner, Alexandra Pope, Jorge A. Zavala, Daisuke Iono, Ryan Cybulski, Miguel Chavez, Daniel Ferrusca, Mark Gurwell, Hansung Gim, Mark H. Heyer, Tanio Díaz-Santos, Elena Terlevich, D. Rosa González, S. M. Rogstad, Milagros Zeballos, David Sánchez-Arguelles, Neal R. Erickson, Gopal Narayanan
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 454:3485-3499
Measuring redshifted CO line emission is an unambiguous method for obtaining an accurate redshift and total cold gas content of optically faint, dusty starburst systems. Here, we report the first successful spectroscopic redshift determination of AzT
Autor:
Javier R, Goicoechea, D, Teyssier, M, Etxaluze, P F, Goldsmith, V, Ossenkopf, M, Gerin, E A, Bergin, J H, Black, J, Cernicharo, S, Cuadrado, P, Encrenaz, E, Falgarone, A, Fuente, A, Hacar, D C, Lis, N, Marcelino, G J, Melnick, H S P, Müller, C, Persson, J, Pety, M, Röllig, P, Schilke, R, Simon, R L, Snell, J, Stutzki
Publikováno v:
The Astrophysical journal. 812(1)
We present the first ~7.5′×11.5′ velocity-resolved (~0.2 km s−1) map of the [C ii] 158 μm line toward the Orion molecular cloud 1 (OMC 1) taken with the Herschel/HIFI instrument. In combination with far-infrared (FIR) photometric images and v
Autor:
Michael J. Kaufman, Edwin A. Bergin, John E. Howe, Gary J. Melnick, David A. Neufeld, David Hollenbach, Zhong Wang, R. L. Snell
Publikováno v:
The Astrophysical Journal. 620:758-773
We have used the Submillimeter Wave Astronomy Satellite (SWAS) to observe the ground-state 110 → 101 transition of ortho-H2O at 557 GHz in three of the shocked molecular clumps associated with the supernova remnant IC 443. We also observed simultan
Autor:
Volker Tolls, Brian M. Patten, Gisbert Winnewisser, Rudolf Schieder, Gordon Chin, Edwin A. Bergin, Neal R. Erickson, M. L. N. Ashby, Y. F. Zhang, S. C. Kleiner, Zhong Wang, Paul F. Goldsmith, Mark Gurwell, David A. Neufeld, Rene Plume, R. L. Snell, Gary J. Melnick, John Stauffer
Publikováno v:
The Astrophysical Journal Supplement Series. 152:137-162
The Submillimeter Wave Astronomy Satellite (SWAS), which was launched in 1998 December, is a NASA mission dedicated to the study of interstellar chemistry and star formation. SWAS is conducting pointed observations of molecular clouds throughout our
Autor:
Paul F. Goldsmith, V. Tolls, R. L. Snell, E. A. Bergin, David A. Neufeld, Gary J. Melnick, John E. Howe, Di Li
Publikováno v:
The Astrophysical Journal. 576:814-831
We report the tentative detection of molecular oxygen in the interstellar medium. Deep integrations using the Submillimeter Wave Astronomy (SWAS) satellite of the ρ Oph A cloud have resulted in a detection of an emission feature consistent with the
Autor:
Volker Tolls, Gisbert Winnewisser, John Stauffer, Zheng Wang, Gordon Chin, Edwin A. Bergin, M. L. N. Ashby, R. L. Snell, Y. F. Zhang, David A. Neufeld, S. C. Kleiner, Martin Harwit, John M. Carpenter, Paul F. Goldsmith, Rudolf Schieder, David G. Koch, Rene Plume, John E. Howe, Gary J. Melnick, Neal R. Erickson, Brian M. Patten
Publikováno v:
The Astrophysical Journal. 539:L115-L118
We present spectral line profiles for the 557 GHz 110 → 101 ground-state rotational transition of ortho-H216O for 18 Galactic star formation regions observed by the Submillimeter Wave Astronomy Satellite. Water is unambiguously detected in every so
[ITAL]Submillimeter Wave Astronomy Satellite[/ITAL] Observations of Extended Water Emission in Orion
Autor:
Volker Tolls, Brian M. Patten, John R. Stauffer, Zhong Wang, Rudolf Schieder, Edwin A. Bergin, Matthew L. N. Ashby, S. C. Kleiner, Gary J. Melnick, Martin Harwit, Gisbert Winnewisser, John E. Howe, Gordon Chin, Rene Plume, Paul F. Goldsmith, R. L. Snell, Y. F. Zhang, David G. Koch, Neal A. Erickson, David A. Neufeld
Publikováno v:
The Astrophysical Journal. 539:L93-L96
We have used the Submillimeter Wave Astronomy Satellite to map the ground-state 1_{10}-1_{01} transition of ortho-water at 557 GHz in the Orion molecular cloud. Water emission was detected in Orion over an angular extent of about 20 arcmin, or nearly
Autor:
R. L. Snell, Gisbert Winnewisser, Gordon Chin, Rudolf Schieder, Zhong Wang, Neal R. Erickson, John Stauffer, Edwin A. Bergin, Paul F. Goldsmith, Brian M. Patten, Rene Plume, Gary J. Melnick, Martin Harwit, David G. Koch, Volker Tolls, Y. F. Zhang, David A. Neufeld, S. C. Kleiner, John E. Howe, Matthew L. N. Ashby
Publikováno v:
The Astrophysical Journal. 539:L123-L127
We have used the Submillimeter Wave Astronomy Satellite (SWAS) to carry out deep integrations on the NJ = 33 → 12 transition of O2 in a variety of Galactic molecular clouds. We here report no convincing detection in an initial set of observations o