Sammanfattning
We discuss different excitation processes behind the Fe II emission lines in the IUE spectrum of KQ Puppis (Boss 1985), a VV Cephei type of spectroscopic binary. Several pa pers have been published on the subject suggesting a number of processes behind the strong Fe II emission lines. We propose that there are two processes operating: selective photoexcitation by continuum radiation (PCR) from the B-star companion, and photoexcitation by accidental resonance (PAR) by the H Ly alpha radiation field. We suggest excitation channels for each of the Fe II emission lines identified in the spectrum.
Originalspråk | Engelska |
---|---|
Sidor (från-till) | 646-654 |
Antal sidor | 8 |
Tidskrift | Astronomy and Astrophysics |
Volym | 364 |
Nummer | 2 |
Status | Publicerad - 2000 |
Nationell ämneskategori
- Astronomi, astrofysik och kosmologi (10305)