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The most variable VVV sources: eruptive protostars, dipping giants in the nuclear disc and others
Indexado
WoS WOS:001428873000002
DOI 10.1093/MNRAS/STAD3929
Año 2024
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



We have performed a comprehensive search of a VISTA Variables in the Via Lactea (VVV) data base of 9.5 yr light curves for variable sources with Delta K-s >= 4 mag, aiming to provide a large sample of high amplitude eruptive young stellar objects (YSOs) and detect unusual or new types of infrared variable source. We find 222 variable or transient sources in the Galactic bulge and disc, most of which are new discoveries. The sample mainly comprises novae, YSOs, microlensing events, Long Period Variable stars (LPVs), and a few rare or unclassified sources. Additionally, we report the discovery of a significant population of aperiodic late-type giant stars suffering deep extinction events, strongly clustered in the Nuclear Disc of the Milky Way. We suggest that these are metal-rich stars in which radiatively driven mass loss has been enhanced by super-solar metallicity. Among the YSOs, 32/40 appear to be undergoing episodic accretion. Long-lasting YSO eruptions have a typical rise time of similar to 2 yr, somewhat slower than the 6-12 month time-scale seen in the few historical events observed on the rise. The outburst durations are usually at least 5 yr, somewhat longer than many lower amplitude VVV events detected previously. The light curves are diverse in nature, suggesting that multiple types of disc instability may occur. Eight long-duration extinction events are seen wherein the YSO dims for a year or more, attributable to inner disc structure. One binary YSO in NGC 6530 displays periodic extinction events (P=59 d) similar to KH 15D.

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Disciplinas de Investigación



WOS
Astronomy & Astrophysics
Scopus
Sin Disciplinas
SciELO
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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



Ord. Autor Género Institución - País
1 Lucas, P. W. - Univ Hertfordshire - Reino Unido
2 Smith, L. C. Mujer UNIV CAMBRIDGE - Reino Unido
3 Guo, Z. - Univ Hertfordshire - Reino Unido
Universidad de Valparaíso - Chile
Núcleo Milenio de Formación Planetaria - Chile
Universidad Técnica Federico Santa María - Chile
4 Pena, C. Contreras - Seoul Natl Univ - Corea del Sur
5 MINNITI-DEL BARCO, DANTE Hombre Universidad Nacional Andrés Bello - Chile
Vatican Observ - Vaticano
UNIV FED SANTA CATARINA - Brasil
6 Miller, N. - Univ Hertfordshire - Reino Unido
7 Alonso-Garcia, J. - Universidad de Antofagasta - Chile
Instituto Milenio de Astrofísica - Chile
8 Catelan, Marcio Hombre Instituto Milenio de Astrofísica - Chile
Pontificia Universidad Católica de Chile - Chile
9 Borissova, J. - Instituto Milenio de Astrofísica - Chile
10 Saito, R. K. -
11 Kurtev, R. - Universidad de Valparaíso - Chile
Instituto Milenio de Astrofísica - Chile
12 Navarro, M. G. - INAF Osservatorio Astron Roma - Italia
13 Morris, C. - Univ Hertfordshire - Reino Unido
14 Muthu, H. - Univ Hertfordshire - Reino Unido
15 Froebrich, D. - Univ Kent - Reino Unido
16 Ivanov, Valentin Hombre European Southern Observ - Alemania
17 Bayo, A. - European Southern Observ - Alemania
18 Caratti o Garatti, A. - INAF Osservatorio Astron Capodimonte - Italia
19 Sanders, J. L. - UCL - Reino Unido

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Financiamiento



Fuente
CNPq/Brazil
STFC
Fondecyt Project
BASAL Center for Astrophysics and Associated Technologies (CATA)
Ministry for the Economy, Development and Tourism, Programa Iniciativa Cientifica Milenio
Brazilian National Council for Scientific and Technological Development (CNPQ)
California Institute of Technology
Millennium Institute of Astrophysics (MAS)
Science and Technology Facilities Committee (STFC)
ESO Public Survey
ANID/FONDECYT
ANID's Millennium Science Initiative
ANID's Basal
Chilean National Agency for Research and Development (ANID) Basal
INAF-GoG 2022 "NIR-dark Accretion Outbursts in Massive Young Stellar Objects (NAOMY)"
PRIN-MUR 2022

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos



Agradecimiento
We thank the referee for their work to improve this paper. We also thank Mike Kuhn for pointing us to the recent discovery of post-RGB stars and Chiaki Kobayashi for pointing out that a dependence of dust production on metallicity would indicate that the dipping giant stars are O-rich rather than C-rich. We gratefully acknowledge data from the ESO Public Survey programs 179.B-2002 and 198.B-2004 taken with the VISTA telescope and products from the Cambridge Astronomical Survey Unit (CASU) and the Wide Field Astronomy Unit at the Royal Observatory, Edinburgh. This research has made use of the National Aeronautics and Space Administration's Infrared Processing and Analysis Centre (IPAC) Infrared Science Archive, which is funded by the and operated by the California Institute of Technology. We also acknowledge use of NASA's Astrophysics Data System Bibliographic Services and the SIMBAD data base operated at Centre de Donnees astronomiques de Strasbourg (CDS), Strasbourg, France. We also made use of the VizieR catalogue access tool, CDS, Strasbourg, France (DOI: 10.26093/cds/vizier). The original description of the VizieR service was published in 2000, A&AS 143, 23. PWL and ZG acknowledge support by Science and Technology Facilities Committee (STFC) Consolidated Grant ST/R00905/1, and CM was supported by an STFC studentship funded by grant ST/S505419/1. DM gratefully acknowledges support from the Chilean National Agency for Research and Development (ANID) Basal projects ACE210002 and FB210003, from Fondecyt Project No. 1220724, and from Brazilian National Council for Scientific and Technological Development (CNPq) Project 350104/2022-0., the Basal Center for Astrophysics and Associated Technologies (CATA) through grant AFB170002, and the Ministry for the Economy, Development and Tourism, Programa Iniciativa Cientifica Milenio grant IC120009, awarded to the Millennium Institute of Astrophysics (MAS). Support for MC is provided by ANID's Millennium Science Initiative through grant ICN12_009, awarded to the MAS; by ANID/FONDECYT Regular grant 1231637; and by ANID's Basal grant FB210003. RKS acknowledges support from CNPq/Brazil through projects 308298/2022-5, 350104/2022-0 and 421034/2023-8. ACG has been supported by grants PRIN-MUR 2022 20228JPA3A "The path to star and planet formation in the JWST era (PATH)" and INAF-GoG 2022 "NIR-dark Accretion Outbursts in Massive Young stellar objects (NAOMY)".

Muestra la fuente de financiamiento declarada en la publicación.