A Study of the Photometric and Spectroscopic Variations of the Prototypical FU Orionis–type Star V1057 Cyg-Reference-Cited by-同舟云学术

A Study of the Photometric and Spectroscopic Variations of the Prototypical FU Orionis–type Star V1057 Cyg

Published:2021-08-01 Issue:2 Volume:917 Page:80
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Szabó Zs. M.^ORCID,Kóspál Á.^ORCID,Ábrahám P.^ORCID,Park S.^ORCID,Siwak M.^ORCID,Green J. D.^ORCID,Moór A.,Pál A.^ORCID,Acosta-Pulido J. A.^ORCID,Lee J.-E.^ORCID,Cseh B.,Csörnyei G.,Hanyecz O.^ORCID,Könyves-Tóth R.^ORCID,Krezinger M.^ORCID,Kriskovics L.^ORCID,Ordasi A.,Sárneczky K.^ORCID,Seli B.^ORCID,Szakáts R.^ORCID,Szing A.,Vida K.^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/ac04b3/pdf

Reference111 articles.

1. Long-term evolution of FU Orionis objects at infrared wavelengths

2. An UXor among FUors: Extinction-related Brightness Variations of the Young Eruptive Star V582 Aur

3. Estimating Distance from Parallaxes. IV. Distances to 1.33 Billion Stars in Gaia Data Release 2

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