Zobrazeno 1 - 10
of 1 553
pro vyhledávání: '"A, Commercon"'
Autor:
Sanhueza, Patricio, Liu, Junhao, Morii, Kaho, Girart, Josep Miquel, Zhang, Qizhou, Stephens, Ian W., Jackson, James M., Cortes, Paulo C., Koch, Patrick M., Cyganowski, Claudia J., Saha, Piyali, Beuther, Henrik, Zhang, Suinan, Beltran, Maria T., Cheng, Yu, Olguin, Fernando A., Lu, Xing, Choudhury, Spandan, Pattle, Kate, andez-Lopez, Manuel Fern, Hwang, Jihye, Kang, Ji-hyun, Karoly, Janik, Ginsburg, Adam, Lyo, A. -Ran, Taniguchi, Kotomi, Jiao, Wenyu, Eswaraiah, Chakali, Luo, Qiu-yi, Wang, Jia-Wei, Commercon, Benoit, Li, Shanghuo, Xu, Fengwei, Chen, Huei-Ru Vivien, Zapata, Luis A., Chung, Eun Jung, Nakamura, Fumitaka, Panigrahy, Sandhyarani, Sakai, Takeshi
A complete understanding of the initial conditions of high-mass star formation and what processes determine multiplicity require the study of the magnetic field (B-field) in young, massive cores. Using ALMA 250 GHz polarization (0.3" = 1000 au) and A
Externí odkaz:
http://arxiv.org/abs/2412.08790
Autor:
Morbidelli, Alessandro, Marrocchi, Yves, Ahmad, Adnan Ali, Bhandare, Asmita, Charnoz, Sebastien, Commercon, Benoit, Dullemond, Cornellis P., Guillot, Tristan, Hennebelle, Patrick, Lee, Yueh-Ning, Lovascio, Francesco, Marschall, Raphael, Marty, Bernard, Maury, Anaelle, Tamami, Okamoto
Publikováno v:
A&A 691, A147 (2024)
We present a plausible and coherent view of the evolution of the protosolar disk that is consistent with the cosmochemical constraints and compatible with observations of other protoplanetary disks and sophisticated numerical simulations. The evidenc
Externí odkaz:
http://arxiv.org/abs/2409.06342
Recent observations have begun probing the early phases of disc formation, but little data yet exists on disc structure and morphology of Class 0 objects. Using simulations, we are able to lay out predictions of disc morphologies expected in future s
Externí odkaz:
http://arxiv.org/abs/2408.16319
Publikováno v:
A&A 689, A12 (2024)
The presence of kiloparsec-sized bubble structures in both sides of the Galactic plan suggests active phases of Sgr A$^\star$, the central supermassive black hole of the Milky-Way in the last 1-6 Myr. The contribution of such event on the cosmic-ray
Externí odkaz:
http://arxiv.org/abs/2405.18447
Publikováno v:
A&A 687, A90 (2024)
The birth process of circumstellar disks remains poorly constrained due to observational and numerical challenges. Recent numerical works have shown that the small-scale physics, often wrapped into a sub-grid model, play a crucial role in disk format
Externí odkaz:
http://arxiv.org/abs/2404.14496
Autor:
Bhandare, Asmita, Commerçon, Benoît, Laibe, Guillaume, Flock, Mario, Kuiper, Rolf, Henning, Thomas, Mignone, Andrea, Marleau, Gabriel-Dominique
Publikováno v:
A&A 687, A158 (2024)
Signposts of early planet formation are ubiquitous in substructured young discs. Dense, hot and high-pressure regions formed during gravitational collapse process, integral to star formation, facilitate dynamical mixing of dust within the protostella
Externí odkaz:
http://arxiv.org/abs/2404.09257
Autor:
Navarro-Almaida, D., Lebreuilly, U., Hennebelle, P., Fuente, A., Commerçon, B., Gal, R. Le, Wakelam, V., Gerin, M., Riviére-Marichalar, P., Beitia-Antero, L., Ascasibar, Y.
The first hydrostatic core (FHSC) phase is a brief stage in the protostellar evolution that is difficult to detect. Our goal is to characterize the chemical evolution of gas and dust during the formation of the FHSC. Moreover, we are interested in an
Externí odkaz:
http://arxiv.org/abs/2403.01905
Population III (pop III) stars were born in halos characterised by a pristine gas composition. In such a halo, once the gas density reaches n$_{\mathrm{H}} \sim$ 1 cm$^{-3}$, molecular cooling leads to the collapse of the gas and the birth of pop III
Externí odkaz:
http://arxiv.org/abs/2401.16821
Autor:
Lebreuilly, U., Hennebelle, P., Colman, T., Maury, A., Tung, N. -D., Testi, L., Klessen, R., Molinari, S., Commerçon, B., González, M., Pacetti, E., Somigliana, A., Rosotti, G.
Protostellar disks are the product of angular momentum conservation during the protostellar collapse. Understanding their formation is crucial because they are the birthplace of planets and because their formation is tightly related to star formation
Externí odkaz:
http://arxiv.org/abs/2310.19672
Publikováno v:
A&A 680, A23 (2023)
Understanding the collapse of dense molecular cloud cores to stellar densities and the subsequent evolution of the protostar is of importance to model the feedback effects such an object has on its surrounding environment, as well as describing the c
Externí odkaz:
http://arxiv.org/abs/2310.01516