Reduction of the maximum mass-loss rate of OH/IR stars due to unnoticed binary interaction

L. Decin; W. Homan; T. Danilovich; A. de Koter; D. Engels; L. B. F. M. Waters; S. Muller; C. Gielen; D. A. García-Hernández; R. J. Stancliffe; M. Van de Sande; G. Molenberghs; F. Kerschbaum; A. A. Zijlstra; I. El Mellah

doi:10.1038/s41550-019-0703-5

Reduction of the maximum mass-loss rate of OH/IR stars due to unnoticed binary interaction

L. Decin (Korresp. Autor*in), W. Homan, T. Danilovich, A. de Koter, D. Engels, L. B. F. M. Waters, S. Muller, C. Gielen, D. A. García-Hernández, R. J. Stancliffe, M. Van de Sande, G. Molenberghs, F. Kerschbaum, A. A. Zijlstra, I. El Mellah

Institut für Astrophysik

Veröffentlichungen: Beitrag in Fachzeitschrift › Short Communication › Peer Reviewed

Originalsprache	Englisch
Seiten (von - bis)	408-415
Seitenumfang	8
Fachzeitschrift	Nature Astronomy
Jahrgang	3
Ausgabenummer	5
DOIs	https://doi.org/10.1038/s41550-019-0703-5
Publikationsstatus	Veröffentlicht - Mai 2019

ÖFOS 2012

103003 Astronomie
103004 Astrophysik

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10.1038/s41550-019-0703-5

http://adsabs.harvard.edu/abs/2019NatAs...3..408D

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Decin, L., Homan, W., Danilovich, T., de Koter, A., Engels, D., Waters, L. B. F. M., Muller, S., Gielen, C., García-Hernández, D. A., Stancliffe, R. J., Van de Sande, M., Molenberghs, G., Kerschbaum, F., Zijlstra, A. A., & El Mellah, I. (2019). Reduction of the maximum mass-loss rate of OH/IR stars due to unnoticed binary interaction. Nature Astronomy, 3(5), 408-415. https://doi.org/10.1038/s41550-019-0703-5

@article{acf41161066b44f88e22b391401614dd,

title = "Reduction of the maximum mass-loss rate of OH/IR stars due to unnoticed binary interaction",

keywords = "AGB STARS, ASYMPTOTIC GIANT BRANCH, DUST, ENVELOPES, EVOLUTION, OH 26.5+0.6, RED SUPERGIANTS, SUPERWIND, WINDS, YIELDS",

author = "L. Decin and W. Homan and T. Danilovich and {de Koter}, A. and D. Engels and Waters, {L. B. F. M.} and S. Muller and C. Gielen and Garc{\'i}a-Hern{\'a}ndez, {D. A.} and Stancliffe, {R. J.} and {Van de Sande}, M. and G. Molenberghs and F. Kerschbaum and Zijlstra, {A. A.} and {El Mellah}, I.",

note = "Publisher Copyright: {\textcopyright} 2019, The Author(s), under exclusive licence to Springer Nature Limited.",

year = "2019",

month = may,

doi = "10.1038/s41550-019-0703-5",

language = "English",

volume = "3",

pages = "408--415",

journal = "Nature Astronomy",

publisher = "NATURE PORTFOLIO",

number = "5",

}

Decin, L, Homan, W, Danilovich, T, de Koter, A, Engels, D, Waters, LBFM, Muller, S, Gielen, C, García-Hernández, DA, Stancliffe, RJ, Van de Sande, M, Molenberghs, G, Kerschbaum, F, Zijlstra, AA & El Mellah, I 2019, 'Reduction of the maximum mass-loss rate of OH/IR stars due to unnoticed binary interaction', Nature Astronomy, Jg. 3, Nr. 5, S. 408-415. https://doi.org/10.1038/s41550-019-0703-5

TY - JOUR

T1 - Reduction of the maximum mass-loss rate of OH/IR stars due to unnoticed binary interaction

AU - Decin, L.

AU - Homan, W.

AU - Danilovich, T.

AU - de Koter, A.

AU - Engels, D.

AU - Waters, L. B. F. M.

AU - Muller, S.

AU - Gielen, C.

AU - García-Hernández, D. A.

AU - Stancliffe, R. J.

AU - Van de Sande, M.

AU - Molenberghs, G.

AU - Kerschbaum, F.

AU - Zijlstra, A. A.

AU - El Mellah, I.

PY - 2019/5

Y1 - 2019/5

KW - AGB STARS

KW - ASYMPTOTIC GIANT BRANCH

KW - DUST

KW - ENVELOPES

KW - EVOLUTION

KW - OH 26.5+0.6

KW - RED SUPERGIANTS

KW - SUPERWIND

KW - WINDS

KW - YIELDS

UR - http://www.scopus.com/inward/record.url?scp=85063188825&partnerID=8YFLogxK

U2 - 10.1038/s41550-019-0703-5

DO - 10.1038/s41550-019-0703-5

M3 - Short communication

VL - 3

SP - 408

EP - 415

JO - Nature Astronomy

JF - Nature Astronomy

IS - 5

ER -

Reduction of the maximum mass-loss rate of OH/IR stars due to unnoticed binary interaction

ÖFOS 2012

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