Abstract
The highly variable young star V2492Cyg (PTF 10nvg; VSX J205126.1+440523) underwent a record peak in brightness in early March 2017, as reported by Ibryamov and Semkov (ATel #10170).
Original language | English |
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Article number | 10259 |
Journal | Astronomer's Telegram |
Publication status | Published - 12 Apr 2017 |
Keywords
- Optical
- Young Stellar Object
- Pre-Main-Sequence Star