ALMA-IMF

Aims. Thanks to the high angular resolution, sensitivity, image fidelity, and frequency coverage of ALMA, we aim to improve our understanding of star formation. One of the breakthroughs expected from ALMA, which is the basis of our Cycle 5 ALMA-IMF Large Program, is the question of the origin of the...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2022-06, Vol.662
Hauptverfasser:	Motte, F, Bontemps, S, Csengeri, T, Pouteau, Y, Louvet, F, Stutz, A M, Cunningham, N, López-Sepulcre, A, Brouillet, N, Galván-Madrid, R, Ginsburg, A, Maud, L, A. Men’shchikov, Nakamura, F, Nony, T, Sanhueza, P, Álvarez-Gutiérrez, R H, Armante, M, Baug, T, Bonfand, M, Busquet, G, Chapillon, E, Díaz-González, D, Fernández-López, M, Guzmán, A E, Herpin, F, H.-L. Liu, Olguin, F, Towner, A P M, Bally, J, Battersby, C, Braine, J, Bronfman, L, H.-R. V. Chen, P. Dell’Ova, J. Di Francesco, González, M, Gusdorf, A, Hennebelle, P, Izumi, N, Joncour, I, Y.-N. Lee, Lefloch, B, Lesaffre, P, X. Lu, Menten, K M, Mignon-Risse, R, Molet, J, Moraux, E, Mundy, L, Q. Nguyen Luong, Reyes, N, Reyes Reyes, S D, J.-F. Robitaille, Rosolowsky, E, Sandoval-Garrido, N A, Schuller, F, Svoboda, B, Tatematsu, K, Thomasson, B, Walker, D, B. Wu, Whitworth, A P, Wyrowski, F
Format:	Artikel
Sprache:	eng
Schlagworte:	Angular resolution Astrochemistry Clouds Complexity Evolution Feedback Filaments Initial mass function Kinematics Molecular gases Protostars Spatial resolution Star & galaxy formation Star clusters Star formation Streamer formation
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