Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Maud LT"'
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⟩
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
https://hal.archives-ouvertes.fr/hal-03043025/file/aa34152-18.pdf
Autor:
Maud, LT, Cesaroni, R, Kumar, MSN, Rivilla, VM, Ginsburg, A, Klaassen, PD, Harsono, D, Sanchez-Monge, A, Ahmadi, A, Allen, V, Beltran, MT, Beuther, H, Galvan-Madrid, R, Goddi, C, Hoare, MG, Hogerheijde, MR, Johnston, KG, Kuiper, R, Moscadelli, L, Peters, T, Testi, L, van der Tak, FFS, de Wit, WJ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=core_ac_uk__::0fb70822cda6dbe320150cad56db7191
https://eprints.whiterose.ac.uk/149932/1/aa35633e-19.pdf
https://eprints.whiterose.ac.uk/149932/1/aa35633e-19.pdf
Autor:
Ahmadi, A, Beuther, H, Mottram, JC, Bosco, F, Linz, H, Henning, T, Winters, JM, Kuiper, R, Pudritz, R, Sánchez-Monge, Á, Keto, E, Beltran, M, Bontemps, S, Cesaroni, R, Csengeri, T, Feng, S, Galvan-Madrid, R, Johnston, KG, Klaassen, P, Leurini, S, Longmore, SN, Lumsden, S, Maud, LT, Menten, KM, Moscadelli, L, Motte, F, Palau, A, Peters, T, Ragan, SE, Schilke, P, Urquhart, JS, Wyrowski, F, Zinnecker, H
Context. The fragmentation mode of high-mass molecular clumps and the properties of the central rotating structures surrounding the most luminous objects have yet to be comprehensively characterised. Aims. We study the fragmentation and kinematics of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::4c615e200cc1d1af9a3f5922fc748d37
https://eprints.whiterose.ac.uk/138427/1/aa32548-17.pdf
https://eprints.whiterose.ac.uk/138427/1/aa32548-17.pdf
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).
