Nova Lup 2016 during the X-ray decay phase
Abstract
Nova Lup 2016 (ASASSN-16kt; see ATel #9538, #9539, #8550, #9554, #9587, #9594 and #9644) has been regularly monitored with Swift since the observations published in ATel #10632 that revealed a luminous supersoft X-ray source with a peak XRT count rate of 61.1(+-)0.1 cts/s on 2017/2/22.
- Publication:
-
The Astronomer's Telegram
- Pub Date:
- September 2017
- Bibcode:
- 2017ATel10722....1O
- Keywords:
-
- Nova