› Forums › Variable Stars › Nova in Cas › P Cygni profiles in sodium, what is the cause?
26 September 2020 at 7:07 pm
#583179
John Coffin
Participant
It looks as if there are P Cygni profiles in sodium. Is the sodium interstellar, and if so, what causes the P Cygni profile? Is the emission component due to photoexcitation by UV from the white dwarf or some other mechanism? Thanks.