Search Results - "Rolffs, R"

THE ABUNDANCE, ORTHO/PARA RATIO, AND DEUTERATION OF WATER IN THE HIGH-MASS STAR-FORMING REGION NGC 6334 I by EMPRECHTINGER, M, Lis, D C, Rolffs, R, Schilke, P, Monje, R R, Comito, C, Ceccarelli, C, Neufeld, D A, VAN DER TAK, F F S

“…(ProQuest: ... denotes formulae and/or non-USASCII text omitted) We present Herschel/HIFI observations of 30 transitions of water isotopologues toward the…”
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The physical and chemical structure of Sagittarius B2, I. Three-dimensional thermal dust and free-free continuum modeling on 100 au to 45 pc scales by Schmiedeke, A, Schilke, P, Möller, Th, Sánchez-Monge, Á, Bergin, E, Comito, C, Csengeri, T, Lis, D. C, Molinari, S, Qin, S. -L, Rolffs, R

“…A&A 588, A143 (2016) We model the dust and free-free continuum emission in the high-mass star-forming region Sagittarius B2 in order to reconstruct the…”
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H2CO and CH3OH maps of the Orion Bar photodissociation region by Leurini, S, Parise, B, Schilke, P, Pety, J, Rolffs, R

“…A previous analysis of methanol and formaldehyde towards the Orion Bar concluded that the two molecular species may trace different physical components,…”
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Submillimeter continuum observations of Sagittarius B2 at subarcsecond spatial resolution by Qin, S. -L, Schilke, P, Rolffs, R, Comito, C, Lis, D. C, Zhang, Q

“…We report the first high spatial resolution submillimeter continuum observations of the Sagittarius B2 cloud complex using the Submillimeter Array (SMA). With…”
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The Abundance, Ortho/Para Ratio, and Deuteration of Water in the High-Mass Star Forming Region NGC 6334 I by Emprechtinger, M, Lis, D. C, Rolffs, R, Schilke, P, Monje, R. R, Comito, C, Ceccarelli, C, Neufeld, D. A, van der Tak, F. F. S

“…We present Herschel/HIFI observations of 30 transitions of water isotopologues toward the high-mass star forming region NGC 6334 I. The line profiles of…”
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APEX 1 mm line survey of the Orion Bar by Leurini, S, Rolffs, R, Thorwirth, S, Parise, B, Schilke, P, Comito, C, Wyrowski, F, Güsten, R, Bergman, P, Menten, K. M, Nyman, L. -AA

“…Unbiased molecular line surveys are a powerful tool for analyzing the physical and chemical parameters of astronomical objects and are the only means for…”
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The distribution of water in the high-mass star-forming region NGC 6334I by Emprechtinger, M, Lis, D. C, Bell, T, Phillips, T. G, Schilke, P, Comito, C, Rolffs, R, van der Tak, F, Ceccarelli, C, Aarts, H, Bacmann, A, Baudry, A, Benedettini, M, Bergin, E. A, Blake, G, Boogert, A, Bottinelli, S, Cabrit, S, Caselli, P, Castets, A, Caux, E, Cernicharo, J, Codella, C, Coutens, A, Crimier, N, Demyk, K, Dominik, C, Encrenaz, P, Falgarone, E, Fuente, A, Gerin, M, Goldsmith, P, Helmich, F, Hennebelle, P, Henning, T, Herbst, E, Hily-Blant, P, Jacq, T, Kahane, C, Kama, M, Klotz, A, Kooi, J, Langer, W, Lefloch, B, Loose, A, Lord, S, Lorenzani, A, Maret, S, Melnick, G, Neufeld, D, Nisini, B, Ossenkopf, V, Pacheco, S, Pagani, L, Parise, B, Pearson, J, Risacher, C, Salez, M, Saraceno, P, Schuster, K, Stutzki, J, Tielens, X, van der Wiel, M, Vastel, C, Viti, S, Wakelam, V, Walters, A, Wyrowski, F, Yorke, H

“…We present observations of twelve rotational transitions of H2O-16, H2O-18, and H2O-17 toward the massive star-forming region NGC 6334 I, carried out with…”
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Herschel/HIFI observations of spectrally resolved methylidyne signatures toward the high-mass star-forming core NGC6334I by van der Wiel, M. H. D, van der Tak, F. F. S, Lis, D. C, Bell, T, Bergin, E. A, Comito, C, Emprechtinger, M, Schilke, P, Caux, E, Ceccarelli, C, Baudry, A, Goldsmith, P. F, Herbst, E, Langer, W, Lord, S, Neufeld, D, Pearson, J, Philips, T, Rolffs, R, Yorke, H, Bacmann, A, Benedettini, M, Blake, G. A, Boogert, A, Bottinelli, S, Cabrit, S, Caselli, P, Castets, A, Cernicharo, J, Codella, C, Coutens, A, Crimier, N, Demyk, K, Dominik, C, Encrenaz, P, Falgarone, E, Fuente, A, Gerin, M, Helmich, F, Hennebelle, P, Henning, T, Hily-Blant, P, Jacq, T, Kahane, C, Kama, M, Klotz, A, Lefloch, B, Lorenzani, A, Maret, S, Melnick, G, Nisini, B, Pacheco, S, Pagani, L, Parise, B, Salez, M, Saraceno, P, Schuster, K, Tielens, A. G. G. M, Vastel, C, Viti, S, Wakelam, V, Walters, A, Wyrowski, F, Edwards, K, Zmuidzinas, J, Morris, P, Samoska, L. A, Teyssier, D

“…Astronomy & Astrophysics, 521, L43 (Oct 2010) In contrast to extensively studied dense star-forming cores, little is known about diffuse gas surrounding…”
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Herschel observations of extra-ordinary sources: Detecting spiral arm clouds by CH absorption lines by Qin, S. -L, Schilke, P, Comito, C, Möller, T, Rolffs, R, Müller, H. S. P, Belloche, A, Menten, K. M, Lis, D. C, Phillips, T. G, Bergin, E. A, Bell, T. A, Crockett, N. R, Blake, G. A, Cabrit, S, Caux, E, Ceccarelli, C, Cernicharo, J, Daniel, F, Dubernet, M. -L, Emprechtinger, M, Encrenaz, P, Falgarone, E, Gerin, M, Giesen, T. F, Goicoechea, J. R, Goldsmith, P. F, Gupta, H, Herbst, E, Joblin, C, Johnstone, D, Langer, W. D, Lord, S. D, Maret, S, Martin, P. G, Melnick, G. J, Morris, P, Murphy, J. A, Neufeld, D. A, Ossenkopf, V, Pagani, L, Pearson, J. C, Pérault, M, Plume, R, Salez, M, Schlemmer, S, Stutzki, J, Trappe, N, van der Tak, F. F. S, Vastel, C, Wang, S, Yorke, H. W, Yu, S, Zmuidzinas, J, Boogert, A, Güsten, R, Hartogh, P, Honingh, N, Karpov, A, Kooi, J, Krieg, J. M, Schieder, R, Diez-Gonzalez, M. C, Bachille, R, Martin-Pintado, J, Baechtold, W, Olberg, M, Nordh, L. H, Gill, J. L, Chattopadhyay, G

“…We have observed CH absorption lines ($J=3/2, N=1 \leftarrow J=1/2, N=1$) against the continuum source Sgr~B2(M) using the \textit{Herschel}/HIFI instrument…”
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