Repeating Outbursts from the Young Stellar Object Gaia23bab (=SPICY 97589)

Michael A. Kuhn; Robert A. Benjamin; Emille E. O. Ishida; Rafael S. de Souza; Julien Peloton; Michele Delli Veneri

doi:10.3847/2515-5172/acc4c9

Repeating Outbursts from the Young Stellar Object Gaia23bab (=SPICY 97589)

Michael A. Kuhn
, Robert A. Benjamin
, Emille E. O. Ishida
, Rafael S. de Souza
, Julien Peloton
, Michele Delli Veneri

Research output: Contribution to journal › Article

Abstract

The light curve of Gaia23bab (=SPICY 97589) shows two significant (ΔG > 2 mag) brightening events, one in 2017 and an ongoing event starting in 2022. The source’s quiescent spectral energy distribution indicates an embedded (A V > 5 mag) pre-main-sequence star, with optical accretion emission and mid-infrared disk emission. This characterization is supported by the source’s membership in an embedded cluster in the star-forming cloud DOBASHI 1604 at a distance of 900 ± 45 pc. Thus, the brightening events are probable accretion outbursts, likely of EX Lup-type.

Original language	English
Pages (from-to)	57
Number of pages	1
Journal	Research Notes of the American Astronomical Society
Volume	7
Issue number	3
DOIs	https://doi.org/10.3847/2515-5172/acc4c9
Publication status	Published - 1 Mar 2023

Keywords

340
Stars and Stellar Physics

Access to Document

10.3847/2515-5172/acc4c9Licence: CC BY

Cite this

@article{4c185c4a884249cba89aaa4c59203a69,

title = "Repeating Outbursts from the Young Stellar Object Gaia23bab (=SPICY 97589)",

abstract = "The light curve of Gaia23bab (=SPICY 97589) shows two significant (ΔG > 2 mag) brightening events, one in 2017 and an ongoing event starting in 2022. The source{\textquoteright}s quiescent spectral energy distribution indicates an embedded (A V > 5 mag) pre-main-sequence star, with optical accretion emission and mid-infrared disk emission. This characterization is supported by the source{\textquoteright}s membership in an embedded cluster in the star-forming cloud DOBASHI 1604 at a distance of 900 ± 45 pc. Thus, the brightening events are probable accretion outbursts, likely of EX Lup-type.",

keywords = "340, Stars and Stellar Physics",

author = "Kuhn, \{Michael A.\} and Benjamin, \{Robert A.\} and Ishida, \{Emille E. O.\} and Souza, \{Rafael S. de\} and Julien Peloton and Veneri, \{Michele Delli\}",

note = "{\textcopyright} 2023. The Author(s). Published by the American Astronomical Society. This is an open access article distributed under the Creative Commons Attribution License, to view a copy of the license, see: https://creativecommons.org/licenses/by/4.0/ ",

year = "2023",

month = mar,

day = "1",

doi = "10.3847/2515-5172/acc4c9",

language = "English",

volume = "7",

pages = "57",

journal = "Research Notes of the American Astronomical Society ",

issn = "2515-5172",

publisher = "IOP Publishing",

number = "3",

}

TY - JOUR

T1 - Repeating Outbursts from the Young Stellar Object Gaia23bab (=SPICY 97589)

AU - Kuhn, Michael A.

AU - Benjamin, Robert A.

AU - Ishida, Emille E. O.

AU - Souza, Rafael S. de

AU - Peloton, Julien

AU - Veneri, Michele Delli

N1 - © 2023. The Author(s). Published by the American Astronomical Society. This is an open access article distributed under the Creative Commons Attribution License, to view a copy of the license, see: https://creativecommons.org/licenses/by/4.0/

PY - 2023/3/1

Y1 - 2023/3/1

N2 - The light curve of Gaia23bab (=SPICY 97589) shows two significant (ΔG > 2 mag) brightening events, one in 2017 and an ongoing event starting in 2022. The source’s quiescent spectral energy distribution indicates an embedded (A V > 5 mag) pre-main-sequence star, with optical accretion emission and mid-infrared disk emission. This characterization is supported by the source’s membership in an embedded cluster in the star-forming cloud DOBASHI 1604 at a distance of 900 ± 45 pc. Thus, the brightening events are probable accretion outbursts, likely of EX Lup-type.

AB - The light curve of Gaia23bab (=SPICY 97589) shows two significant (ΔG > 2 mag) brightening events, one in 2017 and an ongoing event starting in 2022. The source’s quiescent spectral energy distribution indicates an embedded (A V > 5 mag) pre-main-sequence star, with optical accretion emission and mid-infrared disk emission. This characterization is supported by the source’s membership in an embedded cluster in the star-forming cloud DOBASHI 1604 at a distance of 900 ± 45 pc. Thus, the brightening events are probable accretion outbursts, likely of EX Lup-type.

KW - 340

KW - Stars and Stellar Physics

U2 - 10.3847/2515-5172/acc4c9

DO - 10.3847/2515-5172/acc4c9

M3 - Article

SN - 2515-5172

VL - 7

SP - 57

JO - Research Notes of the American Astronomical Society

JF - Research Notes of the American Astronomical Society

IS - 3

ER -

Repeating Outbursts from the Young Stellar Object Gaia23bab (=SPICY 97589)

Abstract

Keywords

Access to Document

Fingerprint

Cite this