Zobrazeno 1 - 10
of 18
pro vyhledávání: '"S. C. Kleiner"'
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:
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
Autor:
Paul F. Goldsmith, S. C. Kleiner, Ronald L. Snell, Edwin A. Bergin, Volker Tolls, David A. Neufeld, Rene Plume, Matthew L. N. Ashby, Zhong Wang, David G. Koch, Rudolf Schieder, Martin Harwit, Y. F. Zhang, Gary J. Melnick, John E. Howe, John Stauffer, Brian M. Patten, Gisbert Winnewisser, Gordon Chin, Neal R. Erickson
Publikováno v:
The Astrophysical Journal. 539:L107-L110
We have observed the 110-101 transition of interstellar water vapor near 557 GHz toward the three outflow sources NGC 2071, L1157, and NGC 1333 IRAS 4 using the Submillimeter Wave Astronomy Satellite. In each case, the observations reveal broad emiss
Autor:
Rene Plume, N. R. Erickson, Gisbert Winnewisser, Paul F. Goldsmith, John Stauffer, Volker Tolls, Gordon Chin, David A. Neufeld, Mark Gurwell, David G. Koch, Edwin A. Bergin, Emmanuel Lellouch, R. L. Snell, Y. F. Zhang, S. C. Kleiner, Rudolf Schieder, Gary J. Melnick, Brian M. Patten, Zhong Wang, Martin Harwit, Matthew L. N. Ashby, John E. Howe
Publikováno v:
The Astrophysical Journal. 539:L147-L150
We have used the Submillimeter Wave Astronomy Satellite to carry out observations on Jupiter and Saturn in two bands centered at 489 and 553 GHz. We detect spectrally resolved 557 GHz H2O emission on both planets, constraining for the first time the
Autor:
Gisbert Winnewisser, Gordon Chin, M. L. N. Ashby, Martin Harwit, V. Tolls, David G. Koch, Rene Plume, Y. F. Zhang, Gary J. Melnick, E. A. Bergin, S. C. Kleiner, Rudolf Schieder, David A. Neufeld, P. F. Goldsmith, Neal R. Erickson, Michael J. Kaufman, John Stauffer, D. J. Hollenbach, R. L. Snell, Z. Wang, John E. Howe, B. M. Patten
Publikováno v:
The Astrophysical Journal. 539:L137-L141
We mapped a 13 by 22 pc region in emission from 492 GHz [C I] and, for the first time, 551 GHz ^{13}CO(5-4) in the giant molecular cloud M17SW, using the Submillimeter Wave Astronomy Satellite. The morphologies of the [C I] and ^{13}CO emission are s
Autor:
Neal R. Erickson, Matthew L. N. Ashby, S. C. Kleiner, John E. Howe, Rene Plume, Gisbert Winnewisser, R. L. Snell, David A. Neufeld, Gordon Chin, Volker Tolls, Brian M. Patten, Paul F. Goldsmith, John Stauffer, Gary J. Melnick, Y. F. Zhang, Rudolf Schieder, Martin Harwit, Zhong Wang, Edwin A. Bergin, David G. Koch
Publikováno v:
The Astrophysical Journal. 539:L151-L154
We have detected the 110-101 pure rotational transition of water vapor toward comet C/1999 H1 using the Submillimeter Wave Astronomy Satellite. Over the period 1999 May 19.01-23.69 UT, the average integrated antenna temperature was 1.79 ± 0.03 K km
Autor:
Mark Gurwell, Gary J. Melnick, Volker Tolls, Rene Plume, Martin Harwit, Zhong Wang, David G. Koch, Matthew L. N. Ashby, S. C. Kleiner, Edwin A. Bergin, Paul F. Goldsmith, Y. F. Zhang, David A. Neufeld, John E. Howe, Neal R. Erickson, John Stauffer, Gisbert Winnewisser, Gordon Chin, R. L. Snell, Rudolf Schieder, Brian M. Patten
Publikováno v:
The Astrophysical Journal. 539:L143-L146
We report the first detections of absorption features in the submillimeter spectrum of Mars that are due to the H2O (110-101) and 13CO (5-4) rotational transitions. Observations were obtained over several days near the planet's closest approach to Ea
Autor:
S. C. Kleiner, Volker Tolls, John Stauffer, David G. Koch, Neal R. Erickson, Martin Harwit, Paul F. Goldsmith, John E. Howe, Y. F. Zhang, Brian M. Patten, Rudolf Schieder, Matthew L. N. Ashby, Gisbert Winnewisser, Gordon Chin, Gary J. Melnick, Zhong Wang, Rene Plume, Ronald L. Snell, Edwin A. Bergin, David A. Neufeld
Publikováno v:
The Astrophysical Journal. 539:L87-L91
We have obtained spectra of the rotational ground-state 110-101 556.936 GHz ortho-H216O and 110-101 547.676 GHz ortho-H218O transitions toward Orion BN/KL using the Submillimeter Wave Astronomy Satellite (SWAS). The ortho-H216O spectrum shows strong