Wed, 04/12/2017 - 01:13
On the CVNet page, under 'Activity at a Glance – New outbursts and unusual activity reported in the last 72 hours' – the star V HYA is listed. But VSX describes it was an SRA. Am I missing something or is this star developing into a CV?
Stephen [HSP]
Pukemaru Observatory
New Zealand
Stephen,
It looks like I left a letter out when I edited the page yesterday. Sorry about the confusion. I'll remove it now.
V Hya is indeed a transitory Carbon star but from AGB to a PPN (pre-planetary nebula).
Gary