Zobrazeno 1 - 10
of 74
pro vyhledávání: '"Rolffs, R."'
Autor:
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.
Publikováno v:
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 three-dimensional density and dust temperature distribution, as a crucial input to follow-up studies of the gas velocit
Externí odkaz:
http://arxiv.org/abs/1602.02274
Autor:
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 H_2^{16}O, H_2^{17}O, H_2^{18}O, and HDO show a complex pattern of emission and absorption compon
Externí odkaz:
http://arxiv.org/abs/1212.5169
We report the first high spatial resolution submillimeter continuum observations of the Sagittarius B2 cloud complex using the Submillimeter Array (SMA). With the subarcsecond resolution provided by the SMA, the two massive star-forming clumps Sgr B2
Externí odkaz:
http://arxiv.org/abs/1105.0344
Autor:
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 Herschel/HIFI as part of the guaranteed time key program Chemical HErschel Surveys of Star form
Externí odkaz:
http://arxiv.org/abs/1007.4226
Autor:
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. With the high spectral resolution and wide velocity coverage provided by HIFI, 31 CH absorpt
Externí odkaz:
http://arxiv.org/abs/1007.1867
Autor:
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.
Publikováno v:
Astronomy & Astrophysics, 521, L43 (Oct 2010)
In contrast to extensively studied dense star-forming cores, little is known about diffuse gas surrounding star-forming regions. We study molecular gas in the high-mass star-forming region NGC6334I, which contains diffuse, quiescent components that a
Externí odkaz:
http://arxiv.org/abs/1007.1539
A previous analysis of methanol and formaldehyde towards the Orion Bar concluded that the two molecular species may trace different physical components, methanol the clumpy material, and formaldehyde the interclump medium. To verify this hypothesis,
Externí odkaz:
http://arxiv.org/abs/1001.0894
Autor:
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 obtaining a complete view of the molecular inventory for a given source. The present work stands
Externí odkaz:
http://arxiv.org/abs/astro-ph/0605714
Autor:
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.
We present results from radiative transfer modeling of the continuum emission towards Sagittarius B2 (hereafter Sgr B2). We have developed a radiative transfer framework – Pandora – that employs RADMC-3D (Dullemond 2012) for a self-consistent det
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od________38::feb26b50d4c5b99823fb73ea5f747ecd
https://resolver.caltech.edu/CaltechAUTHORS:20160708-080025018
https://resolver.caltech.edu/CaltechAUTHORS:20160708-080025018
Autor:
Schmiedeke, A., Schilke, P., Möller, Th., Sánchez-Monge, Á., Bergin, E., Comito, C., Csengeri, T., Lis, D., Molinari, S., Qin, S.-L., Rolffs, R.
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 588, pp.A143. ⟨10.1051/0004-6361/201527311⟩
Astronomy and Astrophysics-A&A, 2016, 588, pp.A143. ⟨10.1051/0004-6361/201527311⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 588, pp.A143. ⟨10.1051/0004-6361/201527311⟩
Astronomy and Astrophysics-A&A, 2016, 588, pp.A143. ⟨10.1051/0004-6361/201527311⟩
International audience
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::b2b9d62301b9b6003f7986c1e23508a1
https://hal.archives-ouvertes.fr/hal-02318424
https://hal.archives-ouvertes.fr/hal-02318424