Zobrazeno 1 - 10
of 373
pro vyhledávání: '"Pouteau, P."'
Autor:
Louvet, F., Sanhueza, P., Stutz, A., Men'shchikov, A., Motte, F., Galván-Madrid, R., Bontemps, S., Pouteau, Y., Ginsburg, A., Csengeri, T., Di Francesco, J., Dell'Ova, P., González, M., Didelon, P., Braine, J., Cunningham, N., Thomasson, B., Lesaffre, P., Hennebelle, P., Bonfand, M., Gusdorf, A., Álverez-Gutiérrez, R. H., Nony, T., Busquet, G., Olguin, F., Bronfman, L., Salinas, J., Fernandez-Lopez, M., Moraux, E., Liu, H. L., Lu, X., Huei-Ru, V., Towner, A., Valeille-Manet, M., Brouillet, N., Herpin, F., Lefloch, B., Baug, T., Maud, L., Lopez-Sepulcre, A., Svodoba, B.
Publikováno v:
A&A 690, A33 (2024)
The stellar initial mass function (IMF) is critical to our understanding of star formation and the effects of young stars on their environment. On large scales, it enables us to use tracers such as UV or Halpha emission to estimate the star formation
Externí odkaz:
http://arxiv.org/abs/2407.18719
Autor:
Dell'Ova, P., Motte, F., Gusdorf, A., Pouteau, Y., Men'shchikov, A., Diaz-Gonzalez, D., Galván-Madrid, R., Lesaffre, P., Didelon, P., Stutz, A. M., Towner, A. P. M., Marsh, K., Whitworth, A., Armante, M., Bonfand, M., Nony, T., Valeille-Manet, M., Bontemps, S., Csengeri, T., Cunningham, N., Ginsburg, A., Louvet, F., Alvarez-Gutierrez, R. H., Brouillet, N., Salinas, J., Sanhueza, P., Nakamura, F., Luong, Q. Nguyen, Baug, T., Fernandez-Lopez, M., Liu, H. -L., Olguin, F.
A crucial aspect in addressing the challenge of measuring the core mass function, that is pivotal for comprehending the origin of the initial mass function, lies in constraining the temperatures of the cores. We aim to measure the luminosity, mass, c
Externí odkaz:
http://arxiv.org/abs/2407.07610
Autor:
Bonfand, M., Csengeri, T., Bontemps, S., Brouillet, N., Motte, F., Louvet, F., Ginsburg, A., Cunningham, N., Galván-Madrid, R., Herpin, F., Wyrowski, F., Valeille-Manet, M., Stutz, A. M., Di Francesco, J., Gusdorf, A., Fernández-López, M., Lefloch, B., Liu, H-L., Sanhueza, P., Álvarez-Gutiérrez, R. H., Olguin, F., Nony, T., Lopez-Sepulcre, A., Dell'Ova, P., Pouteau, Y., Jeff, D., Chen, H. -R. V., Armante, M., Towner, A., Bronfman, L., Kessler, N.
Publikováno v:
A&A 687, A163 (2024)
Sites associated with high-mass star and cluster formation exhibit a so-called hot core phase, characterized by high temperatures and column densities of complex organic molecules. We built a comprehensive census of hot core candidates towards the AL
Externí odkaz:
http://arxiv.org/abs/2402.15023
Autor:
Armante, M., Gusdorf, A., Louvet, F., Motte, F., Pouteau, Y., Lesaffre, P., Galván-Madrid, R., Dell'Ova, P., Bonfand, M., Nony, T., Brouillet, N., Cunningham, N., Ginsburg, A., Men'shchikov, A., Bontemps, S., González, D. Díaz, Csengeri, T., Fernández-López, M., González, M., Herpin, F., Liu, H. -L., Sanhueza, P., Stutz, A. M., Valeille-Manet, M.
Publikováno v:
A&A 686, A122 (2024)
We aimed to measure the CMF in the evolved W33-Main star-forming protocluster to compare it with CMF recently obtained in other Galactic star-forming regions, including the ones included in the ALMA-IMF program. We used observations from the ALMA-IMF
Externí odkaz:
http://arxiv.org/abs/2401.09203
Autor:
Cunningham, N., Ginsburg, A., Galván-Madrid, R., Motte, F., Csengeri, T., Stutz, A. M., Fernández-López, M., Álvarez-Gutiérrez, R. H., Armante, M., Baug, T., Bonfand, M., Bontemps, S., Braine, J., Brouillet, N., Busquet, G., Díaz-González, D. J., Di Francesco, J., Gusdorf, A., Herpin, F., Liu, H., López-Sepulcre, A., Louvet, F., Lu, X., Maud, L., Nony, T., Olguin, F. A., Pouteau, Y., Rivera-Soto, R., Sandoval-Garrido, N. A., Sanhueza, P., Tatematsu, K., Towner, A. P. M., Valeille-Manet, M.
Publikováno v:
A&A 678, A194 (2023)
ALMA-IMF is an Atacama Large Millimeter/submillimeter Array (ALMA) Large Program designed to measure the core mass function (CMF) of 15 protoclusters chosen to span their early evolutionary stages. It further aims to understand their kinematics, chem
Externí odkaz:
http://arxiv.org/abs/2306.14710
Autor:
Nony, T., Galvan-Madrid, R., Motte, F., Pouteau, Y., Cunningham, N., Louvet, F., Stutz, A. M., Lefloch, B., Bontemps, S., Brouillet, N., Ginsburg, A., Joncour, I., Herpin, F., Sanhueza, P., Csengeri, T., Towner, A. P. M., Bonfand, M., Fernández-López, M., Baug, T., Bronfman, L., Busquet, G., Di Francesco, J., Gusdorf, A., Lu, X., Olguin, F., Valeille-Manet, M., Whitworth, A. P.
Publikováno v:
A&A 674, A75 (2023)
The origin of the stellar initial mass function (IMF) and its relation with the core mass function (CMF) are actively debated issues with important implications in astrophysics. Recent observations in the W43 molecular complex of top-heavy CMFs, with
Externí odkaz:
http://arxiv.org/abs/2301.07238
Autor:
Pouteau, Y., Motte, F., Nony, T., Gonzalez, M., Joncour, I., Robitaille, J. -F., Busquet, G., Galvan-Madrid, R., Gusdorf, A., Hennebelle, P., Ginsburg, A., Csengeri, T., Sanhueza, P., Dell'Ova, P., Stutz, A. M., Towner, A. P. M., Cunningham, N., Louvet, F., Men'shchikov, A., Fernandez-Lopez, M., Schneider, N., Armante, M., Bally, J., Baug, T., Bonfand, M., Bontemps, S., Bronfman, L., Brouillet, N., Diaz-Gonzalez, D., Herpin, F., Lefloch, B., Liu, H. -L., Lu, X., Nakamura, F., Luong, Q. Nguyen, Olguin, F., Tatematsu, K., Valeille-Manet, M.
Publikováno v:
A&A 674, A76 (2023)
Among the most central open questions regarding the initial mass function (IMF) of stars is the impact of environment on the shape of the core mass function (CMF) and thus potentially on the IMF. The ALMA-IMF Large Program aims to investigate the var
Externí odkaz:
http://arxiv.org/abs/2212.09307
Autor:
Brouillet, N., Despois, D., Molet, J., Nony, T., Motte, F., Gusdorf, A., Louvet, F., Bontemps, S., Herpin, F., Bonfand, M., Csengeri, T., Ginsburg, A., Cunningham, N., Galvan-Madrid, R., Maud, L., Busquet, G., Bronfman, L., Fernandez-Lopez, M., Jeff, D. L., Lefloch, B., Pouteau, Y., Sanhueza, P., Stutz, A. M., Valeille-Manet, M.
Publikováno v:
A&A 665, A140 (2022)
W43-MM1 is a young region, very rich in terms of high-mass star formation. We aim to systematically identify the massive cores which contain a hot core and compare their molecular composition. We used ALMA high-spatial resolution (2500 au) data of W4
Externí odkaz:
http://arxiv.org/abs/2207.03537
Publikováno v:
A&A 665, A119 (2022)
The spatial properties of small star-clusters suggest that they may originate from a fragmentation cascade of the cloud for which there might be traces up to a few dozen of kAU. Our goal is to investigate the multi-scale spatial structure of gas clum
Externí odkaz:
http://arxiv.org/abs/2206.01154
Autor:
Pouteau, Y., Motte, F., Nony, T., Galván-Madrid, R., Men'shchikov, A., Bontemps, S., Robitaille, J. -F., Louvet, F., Ginsburg, A., Herpin, F., López-Sepulcre, A., Dell'Ova, P., Gusdorf, A., Sanhueza, P., Stutz, A. M., Brouillet, N., Thomasson, B., Armante, M., Baug, T., Busquet, G., Csengeri, T., Cunningham, N., Fernández-López, M., Liu, H. -L., Olguin, F., Towner, A. P. M., Bally, J., Braine, J., Bronfman, L., Joncour, I., González, M., Hennebelle, P., Lu, X., Menten, K. M., Moraux, E., Tatematsu, K., Walker, D., Whitworth, A. P.
Publikováno v:
A&A 664, A26 (2022)
The ALMA-IMF Large Program observed the W43-MM2-MM3 ridge, whose 1.3mm and 3mm ALMA 12m array continuum images reach a 2500au spatial resolution. We used both the best-sensitivity and the line-free ALMA-IMF images, reduced the noise with the multi-re
Externí odkaz:
http://arxiv.org/abs/2203.03276