GMRT observations of the recurrent nova V3890 Sagittarii
Abstract
We report radio observations of the V3890 Sgr obtained using the GMRT at 1.4 GHz and 610 MHz. The radio emission from the source was detected at 1.4 GHz with a strength of 17.0 (4.3) mJy on 2019 September 6.54 UT suggesting the presence of thermal emission.
- Publication:
-
The Astronomer's Telegram
- Pub Date:
- September 2019
- Bibcode:
- 2019ATel13092....1P
- Keywords:
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- Nova