The Outbursting YSOs Catalogue (OYCAT)


Por: Peña, CC, Lee, JE, Herczeg, G, Johnstone, D, Abrahám, P, Antoniucci, S, Audard, M, Ashraf, M, Baek, G, Garatti, AC, Carvalho, A, Cieza, L, Miera, FCSD, Eislöffel, J, Froebrich, D, Giannini, T, Green, J, Ghosh, A, Guo, Z, Hillenbrand, L, Hodapp, K, Jheonn, H, Jose, J, Kim, YJ, Kóspál, A, Lee, HG, Lucas, PW, Magakian, T, Nagy, Z, Naylor, T, Ninan, JP, Peneva, S, Reipurth, B, Scholz, A, Semkov, E, Sicilia-Aguilar, A, Singh, K, Siwak, M, Stecklum, B, Szabó, ZM, Wolf, V, Yoon, SY

Publicada: 1 jul 2025
Resumen:
Young stellar objects (YSOs) can display unpredictable and high-amplitude rises in brightness that can last from a few months to possibly over 100 years. These types of outbursts are explained by large changes in the mass accretion rate from the disk onto the central star. This type of variability has given support to a model of star formation (episodic accretion) where stars would spend most of their lifetimes accreting at low rates, and gain most of their mass through these short-lived accretion outbursts. The universality of episodic accretion, as well as its potential impact on stellar and planetary formation are still under debate. Improvement on the statistics of the members of the eruptive class is needed to better understand the episodic accretion phenomenon and its universality across different mass regimes and environments. In this paper we collect published information on the spectroscopic and photometric characteristics of 174 YSOs confirmed to belong to the eruptive variable class. We classify these objects into five different sub-classes (we find 49 FUor, 20 FUor-like, 16 EX Lupi-type, 81 Peculiar/V1647 Ori-like/MNors and 8 Periodic YSOs). The classification follows what has been done previously in the literature, and it is not an attempt to redefine these classes. In addition, we present a list of 18 embedded, and 6 massive YSOs, as additional categories of eruptive variable YSOs. Due to the complexity and/or faintness of these systems, it is hard to place them into the original classification scheme of this class of variable YSOs. Finally, we present a separate list of 355 candidate eruptive variable YSOs, which either lack spectroscopic information or the available spectroscopic data is not sufficient for an unambiguous classification. The online catalogue of confirmed and candidate eruptive YSOs will be maintained and updated in the future to serve as an important reference for the star formation community.

Filiaciones:
Peña, CC:
 Seoul Natl Univ, Dept Phys & Astron, Seoul 08826, South Korea

 Seoul Natl Univ, Res Inst Basic Sci, Seoul 08826, South Korea

Lee, JE:
 Seoul Natl Univ, Dept Phys & Astron, Seoul 08826, South Korea

Herczeg, G:
 Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China

 Peking Univ, Dept Astron, Beijing 100871, Peoples R China

Johnstone, D:
 NRC Herzberg Astron & Astrophys, Victoria, BC V9E 2E7, Canada

 Univ Victoria, Dept Phys & Astron, Victoria, BC V8P 5C2, Canada

Abrahám, P:
 HUN REN Res Ctr Astron & Earth Sci, MTA Ctr Excellence, Konkoly Observ, H-1121 Budapest, Hungary

 Eotvos Lorand Univ, Inst Phys & Astron, H-1117 Budapest, Hungary

 Univ Vienna, Inst Astron IfA, Turkenschanzstr 17, A-1180 Vienna, Austria

Antoniucci, S:
 INAF Osservatorio Astron Roma, I-00078 Monte Porzio Catone, Italy

Audard, M:
 Univ Geneva, Dept Astron, CH-1290 Versoix, Switzerland

Ashraf, M:
 Indian Inst Sci Educ & Res Tirupati, Dept Phys, Tirupati 517619, Andhra Pradesh, India

Baek, G:
 Seoul Natl Univ, Dept Phys & Astron, Seoul 08826, South Korea

 Seoul Natl Univ, Res Inst Basic Sci, Seoul 08826, South Korea

Garatti, AC:
 INAF Osservatorio Astron Capodimonte, Sal Moiariello 16, I-80131 Naples, Italy

Carvalho, A:
 CALTECH, Dept Astron, MC 249-17, Pasadena, CA 91125 USA

Cieza, L:
 Univ Diego Portales, Fac Ingn & Ciencias, Inst Estudios Astrofis, Santiago 8370191, Chile

 Millennium Nucleus Young Exoplanets & their Moons, Santiago, Chile

Miera, FCSD:
 HUN REN Res Ctr Astron & Earth Sci, MTA Ctr Excellence, Konkoly Observ, H-1121 Budapest, Hungary

 Univ Toulouse, Inst Rech Astrophys & Planetol, UT3 PS, OMP,CNRS, F-31028 Toulouse 4, France

Eislöffel, J:
 Thuringer Landessternwarte Tautenburg, D-07778 Tautenburg, Germany

Froebrich, D:
 Univ Kent, Ctr Astrophys & Planetary Sci, Sch Phys & Astron, Canterbury CT2 7NH, England

Giannini, T:
 INAF Osservatorio Astron Roma, I-00078 Monte Porzio Catone, Italy

Green, J:
 Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA

Ghosh, A:
 Univ Nacl Autonoma Mexico, Inst Radioastron & Astrofis, Morelia 58089, Michoacan, Mexico

Guo, Z:
 Univ Valparaiso, Inst Fis & Astron, Casilla 5030, Valparaiso, Chile

 Nucleo Milenio Formac Planetaria NPF, Casilla 5030, Valparaiso, Chile

 Univ Tecn Feder Santa Maria, Dept Fis, Valparaiso, Chile

Hillenbrand, L:
 CALTECH, Dept Astron, MC 249-17, Pasadena, CA 91125 USA

Hodapp, K:
 Univ Hawaii Manoa, Inst Astron, Hilo, HI 96720 USA

Jheonn, H:
 Seoul Natl Univ, Dept Phys & Astron, Seoul 08826, South Korea

Jose, J:
 Indian Inst Sci Educ & Res Tirupati, Dept Phys, Tirupati 517619, Andhra Pradesh, India

Kim, YJ:
 Seoul Natl Univ, Dept Phys & Astron, Seoul 08826, South Korea

Kóspál, A:
 HUN REN Res Ctr Astron & Earth Sci, MTA Ctr Excellence, Konkoly Observ, H-1121 Budapest, Hungary

 Max Planck Inst Astron, D-69117 Heidelberg, Germany

Lee, HG:
 Korea Astron & Space Sci Inst, Daejeon 34055, South Korea

Lucas, PW:
 Univ Hertfordshire, Ctr Astrophys Res, Coll Lane, Hatfield AL10 9AB, England

Magakian, T:
 Byurakan Observ NAS Armenia, Byurakan 0213, Aragatsotn, Armenia

Nagy, Z:
 HUN REN Res Ctr Astron & Earth Sci, MTA Ctr Excellence, Konkoly Observ, H-1121 Budapest, Hungary

Naylor, T:
 Univ Exeter, Dept Phys & Astron, Exeter EX4 4QL, England

Ninan, JP:
 Tata Inst Fundamental Res, Dept Astron & Astrophys, Mumbai 400005, India

Peneva, S:
 Bulgarian Acad Sci, Inst Astron, Sofia 1784, Bulgaria

 Bulgarian Acad Sci, Natl Astron Observ, Sofia 1784, Bulgaria

Reipurth, B:
 Planetary Sci Inst, Tucson, AZ 85719 USA

Scholz, A:
 Univ St Andrews, Sch Phys & Astron, Scottish Univ Phys Alliance SUPA, St Andrews KY16 9SS, Scotland

Semkov, E:
 Bulgarian Acad Sci, Inst Astron, Sofia 1784, Bulgaria

 Bulgarian Acad Sci, Natl Astron Observ, Sofia 1784, Bulgaria

Sicilia-Aguilar, A:
 Univ Dundee, Sch Sci & Engn, SUPA, Dundee DD1 4HN, Scotland

Singh, K:
 Tata Inst Fundamental Res, Dept Astron & Astrophys, Mumbai 400005, India

Siwak, M:
 Univ Natl Educ Commiss, Mt Suhora Astron Observ, PL-30084 Krakow, Poland

Stecklum, B:
 Thuringer Landessternwarte Tautenburg, D-07778 Tautenburg, Germany

Szabó, ZM:
 HUN REN Res Ctr Astron & Earth Sci, MTA Ctr Excellence, Konkoly Observ, H-1121 Budapest, Hungary

 Univ St Andrews, Sch Phys & Astron, Scottish Univ Phys Alliance SUPA, St Andrews KY16 9SS, Scotland

 Max Planck Inst Radioastron, D-53121 Bonn, Germany

Wolf, V:
 Thuringer Landessternwarte Tautenburg, D-07778 Tautenburg, Germany

Yoon, SY:
 Korea Astron & Space Sci Inst, Daejeon 34055, South Korea
ISSN: 12254614
Editorial
KOREAN ASTRONOMICAL SOCIETY, 61-1 HWA-AM DONG, YUSUNG KU, TAEJON, 305-348, SOUTH KOREA
Tipo de documento: Article
Volumen: 58 Número: 2
Páginas: 209-230
WOS Id: 001586599400001

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