dc.contributor.author | Meyer, DM-A | |
dc.contributor.author | Vorobyov, EI | |
dc.contributor.author | Elbakyan, VG | |
dc.contributor.author | Kraus, S | |
dc.contributor.author | Liu, S-Y | |
dc.contributor.author | Nayakshin, S | |
dc.contributor.author | Sobolev, AM | |
dc.date.accessioned | 2022-10-20T08:55:44Z | |
dc.date.issued | 2022-10-16 | |
dc.date.updated | 2022-10-19T17:35:35Z | |
dc.description.abstract | The burst mode of accretion in massive star formation is a scenario linking
the initial gravitational collapse of parent pre-stellar cores to the
properties of their gravitationally unstable discs and of their
accretion-driven bursts. In this study, we present a series of high-resolution
3D radiation-hydrodynamics numerical simulations for young massive stars formed
out of collapsing 100 Mo molecular cores spinning with several values of the
ratio of rotational-to-gravitational energies beta=5%-9%. The models include
the indirect gravitational potential caused by disc asymmetries. We find that
this modifies the barycenter of the disc, causing significant excursions of the
central star position, which we term stellar wobbling. The stellar wobbling
slows down and protracts the development of gravitational instability in the
disc, reducing the number and magnitude of the accretion-driven bursts
undergone by the young massive stars, whose properties are in good agreement
with that of the burst monitored from the massive protostar M17 MIR. Including
stellar wobbling is therefore important for accurate modeling disc structures.
Synthetic ALMA interferometric images in the millimeter waveband show that the
outcomes of efficient gravitational instability such as spiral arms and gaseous
clumps can be detected for as long as the disc is old enough and has already
entered the burst mode of accretion. | en_GB |
dc.description.sponsorship | Science and Technology Facilities Council (STFC) | en_GB |
dc.description.sponsorship | Ministry of Science and Higher Education of the Russian Federation | en_GB |
dc.description.sponsorship | European Research Council (ERC) | en_GB |
dc.description.sponsorship | MOST | en_GB |
dc.identifier.citation | Published online 16 October 2022 | en_GB |
dc.identifier.doi | 10.1093/mnras/stac2956 | |
dc.identifier.grantnumber | ST/N000757/1 | en_GB |
dc.identifier.grantnumber | 075-15-2020-780 | en_GB |
dc.identifier.grantnumber | 101003096 | en_GB |
dc.identifier.grantnumber | ST/V000721/1 | en_GB |
dc.identifier.grantnumber | 108-2923-M001-006-MY3 | en_GB |
dc.identifier.uri | http://hdl.handle.net/10871/131340 | |
dc.identifier | ORCID: 0000-0001-6017-8773 (Kraus, S) | |
dc.identifier | ScopusID: 24481487500 (Kraus, S) | |
dc.language.iso | en | en_GB |
dc.publisher | Royal Astronomical Society / Oxford University Press | en_GB |
dc.relation.url | http://plutocode.ph.unito.it/ | en_GB |
dc.rights | © 2022 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society | en_GB |
dc.subject | methods: numerical | en_GB |
dc.subject | radiative transfer | en_GB |
dc.subject | stars: circumstellar matter | en_GB |
dc.title | The burst mode of accretion in massive star formation with stellar inertia | en_GB |
dc.type | Article | en_GB |
dc.date.available | 2022-10-20T08:55:44Z | |
dc.identifier.issn | 1365-2966 | |
dc.description | This is the author accepted manuscript. The final version is available from Oxford University Press via the DOI in this record | en_GB |
dc.description | Data availability: This research made use of the PLUTO code developed at the University of Torino by A. Mignone (http://plutocode.ph.unito.it/). The figures have been produced using the Matplotlib plotting library for the Python programming language (https://matplotlib.org/). The data underlying this article will be shared on reasonable request to the corresponding author. | en_GB |
dc.identifier.journal | Monthly Notices of the Royal Astronomical Society | en_GB |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
dc.rights.uri | http://www.rioxx.net/licenses/all-rights-reserved | en_GB |
dcterms.dateSubmitted | 2022-06-23 | |
rioxxterms.version | AM | en_GB |
rioxxterms.licenseref.startdate | 2022-10-16 | |
rioxxterms.type | Journal Article/Review | en_GB |
refterms.dateFCD | 2022-10-19T17:35:41Z | |
refterms.versionFCD | AM | |
refterms.dateFOA | 2022-10-20T08:55:48Z | |
refterms.panel | B | en_GB |