Abstract
In recent years, episodic accretion in young stellar objects (YSOs) has gained increasing relevance and the latest picture of YSO evolution suggests that a large portion of the accreted material is gathered during outbursts. Indeed, most recent observations have corroborated the idea that accretion bursts take place through a broad range of stellar masses, from very low mass to high-mass YSOs and at all stages of star formation. As a matter of fact, episodic accretion has challenged the traditional steady-state accretion model. Here, we review three recently discovered outbursting sources with outstanding characteristics, namely V2775 Ori, V960 Mon, and S255IR NIRS 3.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
