Zobrazeno 1 - 10
of 471
pro vyhledávání: '"Dubreuil, D"'
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:
Kendrew, S., Scheithauer, S., Bouchet, P., Amiaux, J., Azzolini, R., Bouwman, J., Chen, C., Dubreuil, D., Fischer, S., Glasse, A., Greene, T., Lagage, P. -O., Lahuis, F., Ronayette, S., Wright, D., Wright, G. S.
The Low Resolution Spectrometer of the MIRI, which forms part of the imager module, will provide R~100 long-slit and slitless spectroscopy from 5 to 12 micron. The design is optimised for observations of compact sources, such as exoplanet host stars.
Externí odkaz:
http://arxiv.org/abs/1512.03000
Autor:
Bouchet, P., Garcia-Marin, M., Lagage, P. -O., Amiaux, J., Augueres, J. -L., Bauwens, E., Blommaert, J. A. D. L., Chen, C. H., Detre, O. H., Dicken, D., Dubreuil, D., Galdemard, Ph., Gastaud, R., Glasse, A., Gordon, K. D., Gougnaud, F., Guillard, P., Justtanont, K., Krause, O., Leboeuf, D., Longval, Y., Martin, L., Mazy, E., Moreau, V., Olofsson, G., Ray, T. P., Reess, J. -M., Renotte, E., Ressler, M. E., Ronayette, S., Salasca, S., Scheithauer, S., Sykes, J., Thelen, M. P., Wells, M., Wright, D., Wright, G. S.
Publikováno v:
2015 Publications of the Astronomical Society of the Pacific, Volume 127, issue 953, pp.612-622
In this article, we describe the MIRI Imager module (MIRIM), which provides broad-band imaging in the 5 - 27 microns wavelength range for the James Webb Space Telescope. The imager has a 0"11 pixel scale and a total unobstructed view of 74"x113". The
Externí odkaz:
http://arxiv.org/abs/1508.02488
Autor:
Boccaletti, A., Lagage, P. -O., Baudoz, P., Beichman, C., Bouchet, P., Cavarroc, C., Dubreuil, D., Glasse, Alistair, Glauser, A. M., Hines, D. C., Lajoie, C. -P., Lebreton, J., Perrin, M. D., Pueyo, L., Reess, J. M., Rieke, G. H., Ronayette, S., Rouan, D., Soummer, R., Wright, G. S.
Publikováno v:
PASP, 127, 633, 2015
The imaging channel on the Mid-Infrared Instrument (MIRI) is equipped with four coronagraphs that provide high contrast imaging capabilities for studying faint point sources and extended emission that would otherwise be overwhelmed by a bright point-
Externí odkaz:
http://arxiv.org/abs/1508.02352
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:
Guillard, P., Rodet, T., Ronayette, S., Amiaux, J., Abergel, A., Moreau, V., Augueres, J. L., Bensalem, A., Orduna, T., Nehmé, C., Belu, A. R., Pantin, E., Lagage, P. O, Longval, Y., Glasse, A. C. H., Bouchet, P., Cavarroc, C., Dubreuil, D., Kendrew, S.
The Mid Infra Red Instrument (MIRI) is one of the four instruments onboard the James Webb Space Telescope (JWST), providing imaging, coronagraphy and spectroscopy over the 5-28 microns band. To verify the optical performance of the instrument, extens
Externí odkaz:
http://arxiv.org/abs/1006.5735
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
Autor:
Quenette, P. Y., Alonso, M., Chayron, L., Cluzel, P., Dubarry, E., Dubreuil, D., Palazon, S., Pomarol, M.
Publikováno v:
Ursus, 2001 Jan 01. 12, 115-120.
Externí odkaz:
https://www.jstor.org/stable/3873238
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