Dataciencia

Colección SciELO Chile

ALMA resolves the remarkable molecular jet and rotating wind in the extremely radio-quiet galaxy NGC 1377

Indexado

WoS	WOS:000563534900001
Scopus	SCOPUS_ID:85091951995

DOI

10.1051/0004-6361/202038282

Año

2020

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

, implying that the supermassive black hole (SMBH) has a high mass with respect to the stellar velocity dispersion of NGC 1377. We suggest that the SMBH of NGC 1377 is currently in a state of moderate growth, at the end of a more intense phase of accretion and also evolving from a state of more extreme nuclear obscuration. The nuclear growth may be fuelled by low-angular momentum gas inflowing from the gas ejected in the molecular jet and wind. Such a feedback-loop of cyclic outflows and central accretion could explain why there is still a significant reservoir of molecular gas in this ageing, lenticular galaxy. A feedback-loop would be an effective process in growing the nuclear SMBH and thus would constitute an important phase in the evolution of NGC 1377. This also invites new questions as to SMBH growth processes in obscured, dusty galaxies.

Revista

Revista	ISSN
Astronomy & Astrophysics	0004-6361

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Disciplinas de Investigación

WOS
Astronomy & Astrophysics

Scopus
Sin Disciplinas

SciELO
Sin Disciplinas

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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	Aalto, Susanne	Mujer	Chalmers Univ Technol - Suecia Chalmers University of Technology, Onsala Space Observatory - Suecia Onsala Space Observatory - Suecia
2	Falstad, N.	-	Chalmers Univ Technol - Suecia Chalmers University of Technology, Onsala Space Observatory - Suecia Onsala Space Observatory - Suecia
3	Muller, S.	-	Chalmers Univ Technol - Suecia Chalmers University of Technology, Onsala Space Observatory - Suecia
4	Wada, K.	Hombre	KAGOSHIMA UNIV - Japón Kagoshima University - Japón
5	Gallagher, John	Hombre	UNIV WISCONSIN - Estados Unidos University of Wisconsin-Madison - Estados Unidos
6	König, Sabine	-	Chalmers Univ Technol - Suecia Chalmers University of Technology, Onsala Space Observatory - Suecia Onsala Space Observatory - Suecia
7	Sakamoto, K.	Hombre	Acad Sinica - Taiwán Academia Sinica, Institute of Astronomy and Astrophysics - Taiwán
8	Vlemmings, W.	-	Chalmers Univ Technol - Suecia Chalmers University of Technology, Onsala Space Observatory - Suecia
9	Ceccobello, C.	Mujer	Chalmers Univ Technol - Suecia Chalmers University of Technology, Onsala Space Observatory - Suecia Onsala Space Observatory - Suecia
10	Dasyra, K.	Mujer	Univ Athens - Grecia National and Kapodistrian University of Athens - Grecia
11	Combes, Francoise	Mujer	Sorbonne Univ - Francia L'Observatoire de Paris - Francia
12	Garcia-Burillo, S.	Hombre	Observ Madrid - España Observatorio Astronomico Nacional - España
13	Oya, Y.	-	Univ Tokyo - Japón The University of Tokyo - Japón
14	Martin, S.	-	ESO - Chile Atacama Large Millimeter Array - Chile
15	van der Werf, Paul P.	Hombre	Leiden Univ - Países Bajos Leiden Observatory Research Institute - Países Bajos Sterrewacht Leiden - Países Bajos
16	Evans, Aaron S.	Hombre	UNIV VIRGINIA - Estados Unidos NRAO - Estados Unidos University of Virginia - Estados Unidos
17	Kotilainen, J.	Hombre	Univ Turku Quantum - Finlandia Turun yliopisto - Finlandia

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Financiamiento

Fuente
National Science Foundation
Ministry of Science and Technology
European Research Council
MOST
Swedish Research Council
National Aeronautics and Space Administration
Vetenskapsradet
Horizon 2020 Framework Programme
Ministry of Science and Technology, Taiwan
ERC Advanced Grant
NSF grant
Hellenic Foundation for Research and Innovation
MCIU/AEI/FEDER,UE
Hellenic Foundation for Research and Innovation (HFRI)
University of Wisconsin-Madison Foundation
College of Letters Science
College of Letters & Science

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos

Agradecimiento
This paper makes use of the following ALMA data: ADS/JAO.ALMA#2012.1.00900.S. ALMA is a partnership of ESO (representing its Member States), NSF (USA), and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO, and NAOJ. We thank the Nordic ALMA ARC node for excellent support. The Nordic ARC node is funded through Swedish Research Council grant No 2017-00648. S.A. gratefully acknowledges support from an ERC Advanced Grant 789410 and from the Swedish Research Council. K.S. was supported by grant MOST 102-2119-M-001-011-MY3 S.G.B. acknowledges the economic support from grants PGC2018-094671-B-I00 and AYA2016-76682-C3-2-P (MCIU/AEI/FEDER,UE). A.S.E. was supported by NSF grant AST 1816838. J.S.G. thanks the University of Wisconsin-Madison Foundation and College of Letters & Science for partial support of this work. K.M.D. acknowledge financial support by the Hellenic Foundation for Research and Innovation (HFRI), project number 1882. This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.
Acknowledgements. This paper makes use of the following ALMA data: ADS/JAO.ALMA#2012.1.00900.S. ALMA is a partnership of ESO (representing its Member States), NSF (USA), and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO, and NAOJ. We thank the Nordic ALMA ARC node for excellent support. The Nordic ARC node is funded through Swedish Research Council grant No 2017-00648. S.A. gratefully acknowledges support from an ERC Advanced Grant 789410 and from the Swedish Research Council. K.S. was supported by grant MOST 102-2119-M-001-011-MY3 S.G.B. acknowledges the economic support from grants PGC2018-094671-B-I00 and AYA2016-76682-C3-2-P (MCIU/AEI/FEDER,UE). A.S.E. was supported by NSF grant AST 1816838. J.S.G. thanks the University of Wisconsin-Madison Foundation and College of Letters & Science for partial support of this work. K.M.D. acknowledge financial support by the Hellenic Foundation for Research and Innovation (HFRI), project number 1882. This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.

Agradecimiento

This paper makes use of the following ALMA data: ADS/JAO.ALMA#2012.1.00900.S. ALMA is a partnership of ESO (representing its Member States), NSF (USA), and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO, and NAOJ. We thank the Nordic ALMA ARC node for excellent support. The Nordic ARC node is funded through Swedish Research Council grant No 2017-00648. S.A. gratefully acknowledges support from an ERC Advanced Grant 789410 and from the Swedish Research Council. K.S. was supported by grant MOST 102-2119-M-001-011-MY3 S.G.B. acknowledges the economic support from grants PGC2018-094671-B-I00 and AYA2016-76682-C3-2-P (MCIU/AEI/FEDER,UE). A.S.E. was supported by NSF grant AST 1816838. J.S.G. thanks the University of Wisconsin-Madison Foundation and College of Letters & Science for partial support of this work. K.M.D. acknowledge financial support by the Hellenic Foundation for Research and Innovation (HFRI), project number 1882. This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.

Acknowledgements. This paper makes use of the following ALMA data: ADS/JAO.ALMA#2012.1.00900.S. ALMA is a partnership of ESO (representing its Member States), NSF (USA), and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO, and NAOJ. We thank the Nordic ALMA ARC node for excellent support. The Nordic ARC node is funded through Swedish Research Council grant No 2017-00648. S.A. gratefully acknowledges support from an ERC Advanced Grant 789410 and from the Swedish Research Council. K.S. was supported by grant MOST 102-2119-M-001-011-MY3 S.G.B. acknowledges the economic support from grants PGC2018-094671-B-I00 and AYA2016-76682-C3-2-P (MCIU/AEI/FEDER,UE). A.S.E. was supported by NSF grant AST 1816838. J.S.G. thanks the University of Wisconsin-Madison Foundation and College of Letters & Science for partial support of this work. K.M.D. acknowledge financial support by the Hellenic Foundation for Research and Innovation (HFRI), project number 1882. This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.