From clump to disc scales in W3 IRS4

Autor: Mottram, JC, Beuther, H, Ahmadi, A, Klaassen, PD, Beltrán, MT, Csengeri, T, Feng, S, Gieser, C, Henning, T, Johnston, KG, Kuiper, R, Leurini, S, Linz, H, Longmore, SN, Lumsden, S, Maud, LT, Moscadelli, L, Palau, A, Peters, T, Pudritz, RE, Ragan, SE, Sánchez-Monge, Á, Semenov, D, Urquhart, JS, Winters, JM, Zinnecker, H

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 636, pp.A118. ⟨10.1051/0004-6361/201834152⟩

Context. High-mass star formation typically takes place in a crowded environment, with a higher likelihood of young forming stars affecting and being affected by their surroundings and neighbours, as well as links between different physical scales af

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::067ad4ee4d8d89585d7c4ca7be2cb269
https://hal.archives-ouvertes.fr/hal-03043025/file/aa34152-18.pdf

A case study of the IRAM NOEMA large program CORE

Autor: Bosco, F, Beuther, H, Ahmadi, A, Mottram, JC, Kuiper, R, Linz, H, Maud, L, Winters, JM, Henning, T, Feng, S, Peters, T, Semenov, D, Klaassen, PD, Schilke, P, Urquhart, JS, Beltrán, MT, Lumsden, SL, Leurini, S, Moscadelli, L, Cesaroni, R, Sánchez-Monge, Á, Palau, A, Pudritz, R, Wyrowski, F, Longmore, S

Publikováno v: Astronomy & Astrophysics

Context: The formation process of high-mass stars (>8 M⊙) is poorly constrained, particularly the effects of clump fragmentation creating multiple systems and the mechanism of mass accretion onto the cores. Aims: We study the fragmentation of dense

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::b7a5252b706a386f024cd2f8f26e9b1d

A probable Keplerian disk feeding an optically revealed massive young star.

Autor: McLeod AF; Centre for Extragalactic Astronomy, Department of Physics, Durham University, Durham, UK. anna.mcleod@durham.ac.uk.; Institute for Computational Cosmology, Department of Physics, University of Durham, Durham, UK. anna.mcleod@durham.ac.uk., Klaassen PD; UK Astronomy Technology Centre, Royal Observatory, Edinburgh, Edinburgh, UK., Reiter M; Department of Physics and Astronomy, Rice University, Houston, TX, USA., Henshaw J; Astrophysics Research Institute, Liverpool John Moores University, Liverpool, UK.; Max Planck Institute for Astronomy, Heidelberg, Germany., Kuiper R; Faculty of Physics, University of Duisburg-Essen, Duisburg, Germany., Ginsburg A; Department of Astronomy, University of Florida, Gainesville, FL, USA.

Publikováno v: Nature [Nature] 2024 Jan; Vol. 625 (7993), pp. 55-59. Date of Electronic Publication: 2023 Nov 29.

The winds from HL Tau.

Autor: Klaassen PD; UK Astronomy Technology Centre, Royal Observatory Edinburgh, Blackford Hill, Edinburgh EH9 3HJ, UK., Mottram JC; Leiden Observatory, Leiden University, PO Box 9513, NL-2300 RA Leiden, the Netherlands; Max-Planck Institute for Astronomy, Königstuhl 17, D-69117 Heidelberg, Germany., Maud LT; Leiden Observatory, Leiden University, PO Box 9513, NL-2300 RA Leiden, the Netherlands., Juhasz A; Institute of Astronomy, Madingley Road, Cambridge CB3 OHA, UK.

Publikováno v: Monthly notices of the Royal Astronomical Society [Mon Not R Astron Soc] 2016 Apr 28; Vol. 460 (1), pp. 627-633. Date of Electronic Publication: 2016 Apr 28 (Print Publication: 2016).