Zobrazeno 1 - 10
of 426
pro vyhledávání: '"PEARSON, J. C."'
Autor:
Tahani, K., Plume, R., Bergin, E. A., Tolls, V., Phillips, T. G., Caux, E., Cabrit, S., Goicoechea, J. R., Goldsmith, P. F., Johnstone, D., Lis, D. C., Pagani, L., Menten, K. M., Muller, H. S. P., Ossenkopf-Okada, V., Pearson, J. C., van der Tak, F. F. S.
Publikováno v:
ApJ 832, 12 (2016)
We present results from a comprehensive submillimeter spectral survey toward the source Orion South, based on data obtained with the HIFI instrument aboard the \textit{Herschel Space Observatory}, covering the frequency range 480 to 1900 GHz. We dete
Externí odkaz:
http://arxiv.org/abs/1608.06320
Publikováno v:
A&A 586, A17 (2016)
Methyl cyanide is an important trace molecule in space, especially in star-forming regions where it is one of the more common molecules used to derive kinetic temperatures. We want to obtain accurate spectroscopic parameters of minor isotopologs of m
Externí odkaz:
http://arxiv.org/abs/1512.05271
Autor:
Lis, D. C., Schilke, P., Bergin, E. A., Gerin, M., Black, J. H., Comito, C., De Luca, M., Godard, B., Higgins, R., Petit, F. Le, Pearson, J. C., Pellegrini, E. W., Phillips, T. G., Yu, S.
We present new observations of the (6,6) and (9,9) inversion transitions of the hydronium ion toward Sagittarius B2(N) and W31C. Sensitive observations toward Sagittarius B2(N) show that the high, ~ 500 K, rotational temperatures characterizing the p
Externí odkaz:
http://arxiv.org/abs/1403.1207
Autor:
Persson, C. M., De Luca, M., Mookerjea, B., Olofsson, A. O. H., Black, J. H., Gerin, M., Herbst, E., Bell, T. A., Coutens, A., Godard, B., Goicoechea, J. R., Hassel, G. E., Hily-Blant, P., Menten, K. M., Muller, H. S. P, Pearson, J. C., Yu, S.
Publikováno v:
Astronomy & Astrophysics, 2012, 543, 145
We have used the Herschel-HIFI instrument to observe interstellar nitrogen hydrides along the sight-lines towards W49N and G10.6-0.4 in order to elucidate the production pathways leading to nitrogen-bearing species in diffuse gas. All detections show
Externí odkaz:
http://arxiv.org/abs/1208.3979
Autor:
De Beck, E., Lombaert, R., Agúndez, M., Daniel, F., Decin, L., Cernicharo, J., Müller, H. S. P., Min, M., Royer, P., Vandenbussche, B., de Koter, A., Waters, L. B. F. M., Groenewegen, M. A. T., Barlow, M. J., Guélin, M., Kahane, C., Pearson, J. C., Encrenaz, P., Szczerba, R., Schmidt, M. R.
Publikováno v:
Astron. Astrophys. 539 (2012) A108
The C-rich AGB star IRC+10216 undergoes strong mass loss, and quasi-periodic density enhancements in the circumstellar matter have been reported. CO is ubiquitous in the CSE, while CCH emission comes from a spatially confined shell. With the IRAM 30m
Externí odkaz:
http://arxiv.org/abs/1201.1850
Autor:
Müller, H. S. P., Cernicharo, J., Agúndez, M., Decin, L., Encrenaz, P., Pearson, J. C., Teyssier, D., Waters, L. B. F. M.
Publikováno v:
J. Mol. Spectrosc. 271 (2012) 50 - 55
A molecular line survey has been carried out toward the carbon-rich asymptotic giant branch star CW Leo employing the HIFI instrument on board of the Herschel satellite. Numerous features from 480 GHz to beyond 1100 GHz could be assigned unambiguousl
Externí odkaz:
http://arxiv.org/abs/1112.0106
Autor:
Wang, S., Bergin, E. A., Crockett, N. R., Goldsmith, P. F., Lis, D. C., Pearson, J. C., Schilke, P., Bell, T. A., Comito, C., Blake, G. A., Caux, E., Ceccarelli, C., Cernicharo, J., Daniel, F., Dubernet, M. -L., Emprechtinger, M., Encrenaz, P., Gerin, M., Giesen, T. F., Goicoechea, J. R., Gupta, H., Herbst, E., Joblin, C., Johnstone, D., Langer, W. D., Latter, W. B., Lord, S. D., Maret, S., Martin, P. G., Melnick, G. J., Menten, K. M., Morris, P., Muller, H. S. P., Murphy, J. A., Neufeld, D. A., Ossenkopf, V., Perault, M., Phillips, T. G., Plume, R., Qin, S. -L., Schlemmer, S., Stutzki, J., Trappe, N., van der Tak, F. F. S., Vastel, C., Yorke, H. W., Yu, S., Zmuidzinas, J.
We have examined methanol emission from Orion KL with of the {\em Herschel}/HIFI instrument, and detected two methanol bands centered at 524 GHz and 1061 GHz. The 524 GHz methanol band (observed in HIFI band 1a) is dominated by the isolated $\Delta$J
Externí odkaz:
http://arxiv.org/abs/1101.0805
Autor:
Gupta, H., Rimmer, P., Pearson, J. C., Yu, S., Herbst, E., Harada, N., Bergin, E. A., Neufeld, D. A., Melnick, G. J., Bachiller, R., Baechtold, W., Bell, T. A., Blake, G. A., Caux, E., Ceccarelli, C., Cernicharo, J., Chattopadhyay, G., Comito, C., Cabrit, S., Crockett, N. R., Daniel, F., Falgarone, E., Diez-Gonzalez, M. C., Dubernet, M. -L., Erickson, N., Emprechtinger, M., Encrenaz, P., Gerin, M., Gill, J. J., Giesen, T. F., Goicoechea, J. R., Goldsmith, P. F., Joblin, C., Johnstone, D., Langer, W. D., Larsson, B., Latter, W. B., Lin, R. H., Lis, D. C., Liseau, R., Lord, S. D., Maiwald, F. W., Maret, S., Martin, P. G., Martin-Pintado, J., Menten, K. M., Morris, P., Müller, H. S. P., Murphy, J. A., Nordh, L. H., Olberg, M., Ossenkopf, V., Pagani, L., Pérault, M., Phillips, T. G., Plume, R., Qin, S. -L., Salez, M., Samoska, L. A., Schilke, P., Schlecht, E., Schlemmer, S., Szczerba, R., Stutzki, J., Trappe, N., van der Tak, F. F. S., Vastel, C., Wang, S., Yorke, H. W., Zmuidzinas, J., Boogert, A., Güsten, R., Hartogh, P., Honingh, N., Karpov, A., Kooi, J., Krieg, J. -M., Schieder, R., Zaal, P.
We report observations of the reactive molecular ions OH$^+$, H$_2$O$^+$, and H$_3$O$^+$ towards Orion KL with Herschel/HIFI. All three $N=1-0$ fine-structure transitions of OH$^+$ at 909, 971, and 1033GHz and both fine-structure components of the do
Externí odkaz:
http://arxiv.org/abs/1009.1450
Autor:
Cernicharo, J., Waters, L. B. F. M., Decin, L., Encrenaz, P., Tielens, A. G. G. M., Agundez, M., De Beck, E., Muller, H. S. P., Goicoechea, J. R., Barlow, M. J., Benz, A., Crimier, N., Daniel, F., Di Giorgio, A. M., Fich, M., Gaier, T., Garcia-Lario, P., De Koter, A., Khouri, T., Liseau, R., Lombaert, R., Erickson, N., Pardo, J. R., Pearson, J. C., Shipman, R., Sanchez-Contreras, C., Teyssier, D.
We present the first results of a high-spectral-resolution survey of the carbon-rich evolved star IRC+10216 that was carried out with the HIFI spectrometer onboard Herschel. This survey covers all HIFI bands, with a spectral range from 488 to 1901GHz
Externí odkaz:
http://arxiv.org/abs/1008.1199
Autor:
Yıldız, U. A., van Dishoeck, E. F., Kristensen, L. E., Visser, R., Jørgensen, J. K., Herczeg, G. J., van Kempen, T. A., Hogerheijde, M. R., Doty, S. D., Benz, A. O., Bruderer, S., Wampfler, S. F., Deul, E., Bachiller, R., Baudry, A., Benedettini, M., Bergin, E., Bjerkeli, P., Blake, G. A., Bontemps, S., Braine, J., Caselli, P., Cernicharo, J., Codella, C., Daniel, F., di Giorgio, A. M., Dominik, C., Encrenaz, P., Fich, M., Fuente, A., Giannini, T., Goicoechea, J. R., de Graauw, Th., Helmich, F., Herpin, F., Jacq, T., Johnstone, D., Larsson, B., Lis, D., Liseau, R., Liu, F. -C., Marseille, M., McCoey, C., Melnick, G., Neufeld, D., Nisini, B., Olberg, M., Parise, B., Pearson, J. C., Plume, R., Risacher, C., Santiago-Garcia, J., Saraceno, P., Shipman, R., Tafalla, M., Tielens, A. G. G. M., van der Tak, F., Wyrowski, F., Dieleman, P., Jellema, W., Ossenkopf, V., Schieder, R., Stutzki, J.
Publikováno v:
A&A HIFI Special Issue, 2010
Herschel-HIFI observations of high-J lines (up to J_u=10) of 12CO, 13CO and C18O are presented toward three deeply embedded low-mass protostars, NGC 1333 IRAS 2A, IRAS 4A, and IRAS 4B, obtained as part of the Water In Star-forming regions with Hersch
Externí odkaz:
http://arxiv.org/abs/1008.0867