Nova Geminourm No. 2

Nova Geminorum No. 2 as a Wolf-Rayet Star.

It has been known for many years that the spectrum of temporary stars or Novae develops in a later stage into a spectrum nearly identical with that of planetary nebulae. First observed in the case of Nova Aurigae of 1891, the same result has been found to hold for all of the temporary stars observed since that time, including the most important Nova of recent years, Nova Persei of 1901. The que...

Early spectroscopic observations of Nova ( V 1494 ) Aquilae 1999 No . 2 ⋆

Low-and medium resolution spectra of the fast nova, Nova (V1494) Aql 1999 No.2 obtained approximately 6, 7, 19 and 28 days after the maximum brightness are presented and discussed. The spectrum covering the whole optical range at day 6 shows the principal plus diffuse-enhanced spectrum. The presence of strong Fe II multiplets with P-Cyg profiles suggest that V1494 Aql belongs to the " Fe II " c...

Cover vol.2, no.2 October 2005

Vol. 8, No. 2 , 2019

cover Vol. 2 No. 1