Zobrazeno 1 - 10
of 427
pro vyhledávání: '"Minier, V."'
Autor:
Tigé, J., Motte, F., Russeil, D., Zavagno, A., Hennemann, M., Schneider, N., Hill, T., Luong, Q. Nguyen, Di Francesco, J., Bontemps, S., Louvet, F., Didelon, P., Konyves, V., André, Ph., Leuleu, G., Bardagi, J., Anderson, L. D., Arzoumanian, D., Benedettini, M., Bernard, J. -P., Elia, D., Figueira, M., Kirk, J., Martin, P. G., Minier, V., Molinari, S., Nony, T., Persi, P., Pezzuto, S., Polychroni, D., Rayner, T., Rivera-Ingraham, A., Roussel, H., Rygl, K., Spinoglio, L., White, G. J.
Publikováno v:
A&A 602, A77 (2017)
To constrain models of high-mass star formation, the Herschel/HOBYS KP aims at discovering massive dense cores (MDCs) able to host the high-mass analogs of low-mass prestellar cores, which have been searched for over the past decade. We here focus on
Externí odkaz:
http://arxiv.org/abs/1703.09839
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:
Schneider, N., Bontemps, S., Motte, F., Blazere, A., Andre, Ph., Anderson, L. D., Arzoumanian, D., Comeron, F., Didelon, P., Di Francesco, J., Duarte-Cabral, A., Guarcello, M. G., Hennemann, M., Hill, T., Konyves, V., Marston, A., Minier, V., Rygl, K. L. J., Roellig, M., Roy, A., Spinoglio, L., Tremblin, P., White, G. J., Wright, N. J.
Publikováno v:
A&A 591, A40 (2016)
The radiative feedback of massive stars on molecular clouds creates pillars, globules and other features at the interface between the HII region and molecular cloud. We present here Herschel observations between 70 and 500 micron of the immediate env
Externí odkaz:
http://arxiv.org/abs/1604.03967
Autor:
Didelon, P., Motte, F., Tremblin, P., Hill, T., Hony, S., Hennemann, M., Hennebelle, P., Anderson, L. D., Galliano, F., Schneider, N., Rayner, T., Rygl, K., Louvet, F., Zavagno, A., Konyves, V., Sauvage, M., Andre, Ph., Bontemps, S., Peretto, N., Griffin, M., Gonzalez, M., Lebouteiller, V., Arzoumanian, D., Benedettini, M., Di Francesco, J., Menshchikov, A., Minier, V ., Luong, Q. Nguyen, Bernard, J. -P., Palmeirim, P., Pezzuto, S., Rivera-Ingraham, A., Russeil, D., Ward-Thompson, D., White, G. J.
Publikováno v:
A&A 584, A4 (2015)
The surroundings of HII regions can have a profound influence on their development, morphology, and evolution. This paper explores the effect of the environment on H II regions in the MonR2 molecular cloud. We aim to investigate the density structure
Externí odkaz:
http://arxiv.org/abs/1510.09175
Autor:
Tremblin, P., Anderson, L. D., Didelon, P., Raga, A. C., Minier, V., Ntormousi, E., Pettitt, A., Pinto, C., Samal, M., Schneider, N., Zavagno, A.
Publikováno v:
A&A 568, A4 (2014)
This work aims at improving the current understanding of the interaction between H ii regions and turbulent molecular clouds. We propose a new method to determine the age of a large sample of OB associations by investigating the development of their
Externí odkaz:
http://arxiv.org/abs/1406.1801
Autor:
Tremblin, P., Schneider, N., Minier, V., Didelon, P., Hill, T., Anderson, L. D., Motte, F., Zavagno, A., André, Ph., Arzoumanian, D., Audit, E., Benedettini, M., Bontemps, S., Csengeri, T., Di Francesco, J., Giannini, T., Hennemann, M., Luong, Q. Nguyen, Marston, A. P., Peretto, N., Rivera-Ingraham, A., Russeil, D., Rygl, K. L. J., Spinoglio, L., White, G. J.
Ionization feedback should impact the probability distribution function (PDF) of the column density around the ionized gas. We aim to quantify this effect and discuss its potential link to the Core and Initial Mass Function (CMF/IMF). We used in a sy
Externí odkaz:
http://arxiv.org/abs/1401.7333
Autor:
Tremblin, P., Minier, V., Schneider, N., Audit, E., Hill, T., Didelon, P., Peretto, N., Arzoumanian, D., Motte, F., Zavagno, A., Bontemps, S., Anderson, L. D., Andre, Ph., Bernard, J. P., Csengeri, T., Di Francesco, J., Elia, D., Hennemann, M., Konyves, V., Marston, A. P., Luong, Q. Nguyen, Rivera-Ingraham, A., Roussel, H., Sousbie, T., Spinoglio, L., White, G. J., Williams, J.
Pillars and globules are present in many high-mass star-forming regions, such as the Eagle nebula (M16) and the Rosette molecular cloud, and understanding their origin will help characterize triggered star formation. The formation mechanisms of these
Externí odkaz:
http://arxiv.org/abs/1311.3664
Autor:
Jackson, J. M., Rathborne, J. M., Foster, J. B., Whitaker, J. S., Sanhueza, P., Claysmith, C., Mascoop, J. L., Wienen, M., Breen, S. L., Herpin, F., Duarte-Cabral, A., Csengeri, T., Longmore, S., Contreras, Y., Indermuehle, B., Barnes, P. J., Walsh, A. J., Cunningham, M. R., Brooks, K. J., Britton, T. R., Voronkov, M. A., Urquhart, J. S., Alves, J., Jordan, C. H., Hill, T., Hoq, S., Finn, S., C., S., Bains, I., Bontemps, S., Bronfman, L., Caswell, J. L., Deharveng, L., Ellingsen, S. P., Fuller, G. A., Garay, G., Green, J. A., Hindson, L., Jones, P. A., Lenfestey, C., Lo, N., Lowe, V., Mardones, D., Menten, K. M., Minier, V., Morgan, L. K., Motte, F., Muller, E., Peretto, N., Purcell, C. R., Schilke, P., Schneider-Bontemps, N., Schuller, F., Titmarsh, A., Wyrowski, F., Zavagno, A.
The Millimetre Astronomy Legacy Team 90 GHz (MALT90) survey aims to characterise the physical and chemical evolution of high-mass star-forming clumps. Exploiting the unique broad frequency range and on-the-fly mapping capabilities of the Australia Te
Externí odkaz:
http://arxiv.org/abs/1310.1131
Autor:
Rivera-Ingraham, A., Martin, P. G., Polychroni, D., Motte, F., Schneider, N., Bontemps, S., Hennemann, M., Menshchikov, A., Luong, Q. Nguyen, Andre, Ph., Arzoumanian, D., Bernard, J. -Ph., Di Francesco, J., Elia, D., Fallscheer, C., Hill, T., Li, J. Z., Minier, V., Pezzuto, S., Roy, A., Rygl, K. L. J., Sadavoy, S. I., Spinoglio, L., White, G. J., Wilson, C. D.
The W3 GMC is a prime target for the study of the early stages of high-mass star formation. We have used Herschel data from the HOBYS key program to produce and analyze column density and temperature maps. Two preliminary catalogs were produced by ex
Externí odkaz:
http://arxiv.org/abs/1301.3805
Autor:
Rygl, K. L. J., Benedettini, M., Schisano, E., Elia, D., Molinari, S., Pezzuto, S., André, Ph., Bernard, J. P., White, G. J., Polychroni, D., Bontemps, S., Cox, N. L. J., Di Francesco, J., Facchini, A., Fallscheer, C., di Giorgio, A. M., Hennemann, M., Hill, T., Könyves, V., Minier, V., Motte, F., Nguyen-Luong, Q., Peretto, N., Pestalozzi, M., Sadavoy, S., Schneider, N., Spinoglio, L., Testi, L., Ward-Thompson, D.
We present a study of the star formation histories of the Lupus I, III, and IV clouds using the Herschel 70-500 micron maps obtained by the Herschel Gould Belt Survey Key Project. By combining the new Herschel data with the existing Spitzer catalog w
Externí odkaz:
http://arxiv.org/abs/1211.5232