New Eruptive YSOs from SPICY and WISE

被引:0
|
作者
Pena, Carlos Contreras [1 ,2 ]
Ashraf, Mizna [3 ]
Lee, Jeong-Eun [1 ,4 ]
Herczeg, Gregory [5 ,6 ]
Lucas, Phil [7 ]
Guo, Zhen [7 ,8 ,9 ,10 ]
Johnstone, Doug [11 ,12 ]
Lee, Ho-Gyu [13 ]
Jose, Jessy [3 ]
机构
[1] Seoul Natl Univ, Dept Phys & Astron, Seoul 08826, South Korea
[2] Seoul Natl Univ, Res Inst Basic Sci, Seoul 08826, South Korea
[3] Indian Inst Sci Educ & Res IISER Tirupati, Tirupati 517507, India
[4] Seoul Natl Univ, SNU Astron Res Ctr, Seoul 08826, South Korea
[5] Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China
[6] Peking Univ, Dept Astron, Beijing 100871, Peoples R China
[7] Univ Hertfordshire, Ctr Astrophys Res, Hatfield AL10 9AB, Herts, England
[8] Univ Valparaiso, Inst Fis & Astron, Casilla 5030, Valparaiso, Chile
[9] Nucleo Milenio Formac Planetaria NPF, Casilla 5030, Valparaiso, Chile
[10] Univ Tecn Federico Santa Maria, Dept Fis, Ave Espana 1680, Valparaiso, Chile
[11] NRC Herzberg Astron & Astrophys, Victoria, BC V9E 2E7, Canada
[12] Univ Victoria, Dept Phys & Astron, Victoria, BC V8P 5C2, Canada
[13] Korea Astron & Space Sci Inst, Taejon 34055, South Korea
基金
英国科学技术设施理事会; 新加坡国家研究基金会; 加拿大自然科学与工程研究理事会;
关键词
stars: pre-main sequence; stars: protostars; stars: variables: T Tauri; Herbig Ae/Be; stars: formation; YOUNG STELLAR OBJECTS; FU ORIONIS OUTBURSTS; EXOR VARIABLES; GALACTIC PLANE; VARIABILITY; CATALOG; HISTORY; SPITZER; UKIDSS; STARS;
D O I
10.5303/JKAS.2023.56.2.253
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This work presents four high-amplitude variable YSOs (similar or equal to 3 mag at near- or mid-IR wavelengths) arising from the SPICY catalog. Three outbursts show a duration that is longer than 1 year, and are still ongoing. And additional YSO brightened over the last two epochs of NEOWISE observations and the duration of the outburst is thus unclear. Analysis of the spectra of the four sources confirms them as new members of the eruptive variable class. We find two YSOs that can be firmly classified as bona fide FUors and one object that falls in the V1647 Ori-like class. Given the uncertainty in the duration of its outburst, an additional YSO can only be classified as a candidate FUor. Continued monitoring and follow-up of these particular sources is important to better understand the accretion process of YSOs.
引用
收藏
页码:253 / 262
页数:10
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