SIMBAD references

2004AJ....128.2962L - Astron. J., 128, 2962-2964 (2004/December-0)

The late appearance of He I in V445 Puppis.

LYNCH D.K., RUDY R.J., MAZUK S., VENTURINI C.C., PUETTER R.C. and PERRY R.B.

Abstract (from CDS):

We present a 0.9-2.5 µm spectrum of V445 Puppis obtained about 3 years after maximum brightness. The spectrum shows thermal continuum emission and two narrow, structured emission lines: He I 1.0830 µm and 2.0581 µm. We interpret this to be emission from a hydrogen-deficient, helium-rich, low-temperature nebula surrounded by an optically thick dust shell, probably carbonaceous.

Abstract Copyright: ∼

Journal keyword(s): ISM: Dust, Extinction - Infrared: Stars - Line: Identification - Stars: Novae, Cataclysmic Variables

Simbad objects: 2

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