Zobrazeno 1 - 10
of 4 397
pro vyhledávání: '"A. Gueth"'
Autor:
Launhardt, R., Pavlyuchenkov, Ya. N., Akimkin, V. V., Dutrey, A., Gueth, F., Guilloteau, S., Henning, Th., Pietu, V., Schreyer, K., Semenov, D., Stecklum, B., Bourke, T. L.
Publikováno v:
A&A 678, A135 (2023)
The disk-outflow connection plays a key role in extracting excess angular momentum from a forming protostar. We have previously reported the discovery of a small molecular outflow from the edge-on T Tauri star in the Bok globule CB26 that shows a pec
Externí odkaz:
http://arxiv.org/abs/2309.01629
Autor:
Yang, Zichen, Wang, Lichen, Laha, Sourav, Zhao, Dong, Luo, Mingdi, Güth, Achim, Taniguchi, Takashi, Watanabe, Kenji, Lotsch, Bettina V., Smet, Jurgen H., Minola, Matteo, Gretarsson, Hlynur, Keimer, Bernhard
We present Ru $L_3$-edge resonant inelastic x-ray scattering (RIXS) measurements of spin-orbit and d-d excitations in exfoliated nanolayers of the Kitaev spin-liquid candidate RuCl$_3$. Whereas the spin-orbit excitations are independent of thickness,
Externí odkaz:
http://arxiv.org/abs/2303.05135
Publikováno v:
In Journal of Economic Behavior and Organization July 2024 223:1-20
Autor:
Podio, L., Tabone, B., Codella, C., Gueth, F., Maury, A., Cabrit, S., Lefloch, B., Maret, S., Belloche, A., André, P., Anderl, S., Gaudel, M., Testi, L.
Publikováno v:
A&A 648, A45 (2021)
As a part of the CALYPSO large programme, we constrain the properties of protostellar jets and outflows in a sample of 21 Class 0 protostars with internal luminosities, Lint, from 0.035 to 47 Lsun. We analyse high angular resolution (~0.5"-1") IRAM P
Externí odkaz:
http://arxiv.org/abs/2012.15379
Publikováno v:
In Journal of Behavioral and Experimental Economics February 2024 108
Autor:
Anderl, S., Maret, S., Cabrit, S., Maury, A. J., Belloche, A., André, Ph., Bacmann, A., Codella, C., Podio, L., Gueth, F.
Context. The process of mass accretion in the earliest phases of star formation is still not fully understood: Does the accretion rate smoothly decline with the age of the protostar or are there short, intermittent accretion bursts? Aims. We aim to e
Externí odkaz:
http://arxiv.org/abs/2011.05979
Autor:
Tabone, B., Cabrit, S., Forêts, G. Pineau des, Ferreira, J., Gusdorf, A., Podio, L., Bianchi, E., Chapillon, E., Codella, C., Gueth, F.
Publikováno v:
A&A 640, A82 (2020)
Large millimeter interferometers are revealing a growing number of rotating outflows, which are suggested to trace magneto-centrifugal disk winds (MHD DWs). However, their impact on disk accretion is not yet well quantified. Here we identify systemat
Externí odkaz:
http://arxiv.org/abs/2004.08804
Autor:
Belloche, A., Maury, A. J., Maret, S., Anderl, S., Bacmann, A., André, Ph., Bontemps, S., Cabrit, S., Codella, C., Gaudel, M., Gueth, F., Lefèvre, C., Lefloch, B., Podio, L., Testi, L.
Publikováno v:
A&A 635, A198 (2020)
Complex organic molecules (COMs) have been detected in a few Class 0 protostars but their origin is not well understood. Going beyond studies of individual objects, we want to investigate the origin of COMs in young protostars on a statistical basis.
Externí odkaz:
http://arxiv.org/abs/2002.00592
Autor:
Maret, S., Maury, A. J., Belloche, A., Gaudel, M., André, Ph., Cabrit, S., Codella, C., Lefèvre, C., Podio, L., Anderl, S., Gueth, F., Hennebelle, P.
Publikováno v:
A&A 635, A15 (2020)
The formation of protoplanetary disks is not well understood. To understand how and when these disks are formed, it is crucial to characterize the kinematics of the youngest protostars at a high angular resolution. Here we study a sample of 16 Class
Externí odkaz:
http://arxiv.org/abs/2001.06355
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