Zobrazeno 1 - 10
of 426
pro vyhledávání: '"Gonzalez, M. C."'
Autor:
Herrera-Yagüe, C., Schneider, C. M., Couronné, T., Smoreda, Z., Benito, R. M., Zufiria, P. J., González, M. C.
The appearance of large geolocated communication datasets has recently increased our understanding of how social networks relate to their physical space. However, many recurrently reported properties, such as the spatial clustering of network communi
Externí odkaz:
http://arxiv.org/abs/1506.00770
Akademický článek
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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:
Rolffs, Rainer, Schilke, Peter, Comito, Claudia, Bergin, E. A., van der Tak, F. F. S., Lis, D. C., Qin, S. -L., Menten, K. M., Guesten, R., Bell, T. A., Blake, G. A., Caux, E., Ceccarelli, C., Cernicharo, J., Crockett, N. R., Daniel, F., Dubernet, M. -L., Emprechtinger, M., Encrenaz, P., Gerin, M., Giesen, T. F., Goicoechea, J. R., Goldsmith, P. F., Gupta, H., Herbst, E., Joblin, C., Johnstone, D., Langer, W. D., Latter, W. D., Lord, S. D., Maret, S., Martin, P. G., Melnick, G. J., Morris, P., Mueller, H. S. P., Murphy, J. A., Ossenkopf, V., Pearson, J. C., Perault, M., Phillips, T. G., Plume, R., Schlemmer, S., Stutzki, J., Trappe, N., Vastel, C., Wang, S., Yorke, H. W., Yu, S., Zmuidzinas, J., Diez-Gonzalez, M. C., Bachiller, R., Martin-Pintado, J., Baechtold, W., Olberg, M., Nordh, L. H., Gill, J. J., Chattopadhyay, G.
To investigate the accretion and feedback processes in massive star formation, we analyze the shapes of emission lines from hot molecular cores, whose asymmetries trace infall and expansion motions. The high-mass star forming region SgrB2(M) was obse
Externí odkaz:
http://arxiv.org/abs/1007.5131
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:
Bujarrabal, V., Alcolea, J., Soria-Ruiz, R., Planesas, P., Teyssier, D., Marston, A. P., Cernicharo, J., Decin, L., Dominik, C., Justtanont, K., de Koter, A., Melnick, G., Menten, K. M., Neufeld, D. A., Olofsson, H., Schmidt, M., Schoier, F. L., Szczerba, R., Waters, L. B. F. M., Quintana-Lacaci, G., Gusten, R., Gallego, J. D., Diez-Gonzalez, M. C., Barcia, A., Lopez-Fernandez, I., Wildeman, K., Tielens, A. G. G. M., Jacobs, K.
We performed Herschel/HIFI observations of several CO lines in the far-infrared/sub-mm in the protoplanetary nebula CRL618. The high spectral resolution provided by HIFI allows measurement of the line profiles. Since the dynamics and structure of the
Externí odkaz:
http://arxiv.org/abs/1007.1570
Autor:
Ossenkopf, V., Röllig, M., Simon, R., Schneider, N., Okada, Y., Stutzki, J., Gerin, M., Akyilmaz, M., Beintema, D., Benz, A. O., Berne, O., Boulanger, F., Bumble, B., Coeur-Joly, O., Dedes, C., Diez-Gonzalez, M. C., France, K., Fuente, A., Gallego, J. D., Goicoechea, J. R., Güsten, R., Harris, A., Higgins, R., Jackson, B., Jarchow, C., Joblin, C., Klein, T., Kramer, C., Lord, S., Martin, P., Martin-Pintado, J., Mookerjea, B., Neufeld, D. A., Phillips, T., Rizzo, J. R., van der Tak, F. F. S., Teyssier, D., Yorke, H.
The molecular gas in the DR21 massive star formation region is known to be affected by the strong UV field from the central star cluster and by a fast outflow creating a bright shock. The relative contribution of both heating mechanisms is the matter
Externí odkaz:
http://arxiv.org/abs/1005.2517
Publikováno v:
Nature 453, 479-482 (2008)
Despite their importance for urban planning, traffic forecasting, and the spread of biological and mobile viruses, our understanding of the basic laws governing human motion remains limited thanks to the lack of tools to monitor the time resolved loc
Externí odkaz:
http://arxiv.org/abs/0806.1256
Publikováno v:
J. Phys. A: Math. Theor. 41 (2008) 224015.
Novel aspects of human dynamics and social interactions are investigated by means of mobile phone data. Using extensive phone records resolved in both time and space, we study the mean collective behavior at large scales and focus on the occurrence o
Externí odkaz:
http://arxiv.org/abs/0710.2939
Publikováno v:
Phys. Rev. E 75, 066108 (2007)
Understanding how opinions spread through a community or how consensus emerges in noisy environments can have a significant impact on our comprehension of social relations among individuals. In this work a model for the dynamics of opinion formation
Externí odkaz:
http://arxiv.org/abs/physics/0701169