Zobrazeno 1 - 10
of 192
pro vyhledávání: '"Pennec, J P"'
Autor:
Schuller, F., André, Ph., Shimajiri, Y., Zavagno, A., Peretto, N., Arzoumanian, D., Csengeri, T., Könyves, V., Palmeirim, P., Pezzuto, S., Rigby, A., Roussel, H., Ajeddig, H., Dumaye, L., Gallais, P., Pennec, J. Le, Martignac, J., Mattern, M., Revéret, V., Rodriguez, L., Talvard, M.
Publikováno v:
A&A 651, A36 (2021)
(abridged) Within the Orion A molecular cloud, the integral-shaped filament (ISF) is a prominent, degree-long structure of dense gas and dust, with clear signs of recent and on-going high-mass star formation. We used the ArTeMiS bolometer camera at A
Externí odkaz:
http://arxiv.org/abs/2104.03717
Akademický článek
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Autor:
André, Ph., Revéret, V., Könyves, V., Arzoumanian, D., Tigé, J., Gallais, P., Roussel, H., Pennec, J. Le, Rodriguez, L., Doumayrou, E., Dubreuil, D., Lortholary, M., Martignac, J., Talvard, M., Delisle, C., Visticot, F., Dumaye, L., De Breuck, C., Shimajiri, Y., Motte, F., Bontemps, S., Hennemann, M., Zavagno, A., Russeil, D., Schneider, N., Palmeirim, P., Peretto, N., Hill, T., Minier, V., Roy, A., Rygl, K. L. J.
Publikováno v:
A&A 592, A54 (2016)
Herschel observations of nearby molecular clouds suggest that interstellar filaments and prestellar cores represent two fundamental steps in the star formation process. The observations support a picture of low-mass star formation according to which
Externí odkaz:
http://arxiv.org/abs/1605.07434
Autor:
Hill, T., Andre, Ph., Arzoumanian, D., Motte, F., Minier, V., Menshchikov, A., Didelon, P., Hennemann, M., Konyves, V., Nguyen-Luong, Q., Palmeirim, P., Peretto, N., Schneider, N., Bontemps, S., Louvet, F., Elia, D., Giannini, T., Reveret, V., Pennec, J. Le, Rodriguez, L., Boulade, O., Doumayrou, E., Dubreuil, D., Gallais, P., Lortholary, M., Martignac, J., Talvard, M., De Breuck, C.
We present APEX/P-ArT\'eMiS 450\mu m continuum observations of RCW 36 and the adjacent ridge, a high-mass high-column density filamentary structure at the centre of the Vela C molecular cloud. These observations, at higher resolution than Herschel's
Externí odkaz:
http://arxiv.org/abs/1211.0275
Autor:
Dannerbauer, H., Daddi, E., Morrison, G. E., Altieri, B., Andreani, P., Aussel, H., Berta, S., Bongiovanni, A., Cava, A., Cepa, J., Cimatti, A., Dominguez, H., Elbaz, D., Schreiber, N. Forster, Genzel, R., Gruppioni, C., Horeau, B., Hwang, H. S., Floc'h, E. Le, Pennec, J. Le, Lutz, D., Magdis, G., Magnelli, B., Maiolino, R., Nordon, R., Garcia, A. M. Perez, Poglitsch, A., Popesso, P., Pozzi, F., Riguccini, L., Rodighiero, G., Saintonge, A., Santini, P., Sanchez-Portal, M., Shao, L., Sturm, E., Tacconi, L., Valtchanov, I.
We present a search for Herschel-PACS counterparts of dust-obscured, high-redshift objects previously selected at submillimeter and millimeter wavelengths in the Great Observatories Origins Deep Survey North field. We detect 22 of 56 submillimeter ga
Externí odkaz:
http://arxiv.org/abs/1007.1902
Autor:
Horeau, B., Claret, A., Rodriguez, L., Billot, N., Boulade, O., Doumayrou, E., Okumura, K., Pennec, J. Le
Publikováno v:
PROCEEDINGS OF THE 9th EUROPEAN WORKSHOP ON RADIATION EFFECTS ON COMPONENTS AND SYSTEMS (RADECS 2006 WORKSHOP) - ATHENS, GREECE, 27-29 SEPTEMBER 2006 Session G: Photonics Devices and Integrated Circuits - PG9
A new concept of bolometer arrays is used for the imager of PACS, one of the three instruments aboard the future Herschel space observatory. Within the framework of PACS photometer characterization, irradiation tests were performed on a dedicated bol
Externí odkaz:
http://arxiv.org/abs/1006.4232
Autor:
André, Ph., Men'shchikov, A., Bontemps, S., Könyves, V., Motte, F., Schneider, N., Didelon, P., Minier, V., Saraceno, P., Ward-Thompson, D., Di Francesco, J., White, G., Molinari, S., Testi, L., Abergel, A., Griffin, M., Henning, Th., Royer, P., Merín, B., Vavrek, R., Attard, M., Arzoumanian, D., Wilson, C. D., Ade, P., Aussel, H., Baluteau, J. -P., Benedettini, M., Bernard, J. -Ph., Blommaert, J. A. D. L., Cambrésy, L., Cox, P., Di Giorgio, A., Hargrave, P., Hennemann, M., Huang, M., Kirk, J., Krause, O., Launhardt, R., Leeks, S., Pennec, J. Le, Li, J. Z., Martin, P., Maury, A., Olofsson, G., Omont, A., Peretto, N., Pezzuto, S., Prusti, T., Roussel, H., Russeil, D., Sauvage, M., Sibthorpe, B., Sicilia-Aguilar, A., Spinoglio, L., Waelkens, C., Woodcraft, A., Zavagno, A.
We summarize the first results from the Gould Belt survey, obtained toward the Aquila Rift and Polaris Flare regions during the 'science demonstration phase' of Herschel. Our 70-500 micron images taken in parallel mode with the SPIRE and PACS cameras
Externí odkaz:
http://arxiv.org/abs/1005.2618
Autor:
Minier, V., André, Ph., Bergman, P., Motte, F., Wyrowski, F., Pennec, J. Le, Rodriguez, L., Boulade, O., Doumayrou, E., Dubreuil, D., Gallais, P., Hamon, G., Lagage, P. -O., Lortholary, M., Martignac, J., Revéret, V., Roussel, H., Talvard, M., Willmann, G., Olofsson, H.
Publikováno v:
Astronomy and Astrophysics 501 (2009) L1-L4
Aims. Expanding HII regions and propagating shocks are common in the environment of young high-mass star-forming complexes. They can compress a pre-existing molecular cloud and trigger the formation of dense cores. We investigate whether these phenom
Externí odkaz:
http://arxiv.org/abs/0907.3031
Autor:
André, P., Minier, V., Gallais, P., Reveret, V., Pennec, J. Le, Rodriguez, L., Boulade, O., Doumayrou, E., Dubreuil, D., Lortholary, M., Martignac, J., Talvard, M., De Breuck, C., Hamon, G., Schneider, N., Bontemps, S., Lagage, P. O., Pantin, E., Roussel, H., Miller, M., Purcell, C. R., Hill, T., Stutzki, J.
Context: The earliest phases of massive star formation are currently much debated. Aims. In an effort to make progress, we took a census of Class0-like protostellar dense cores in the NGC 3576 region, one of the nearest and most luminous embedded sit
Externí odkaz:
http://arxiv.org/abs/0809.3968
Akademický článek
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