Bibcode
Vilchez, J. M.; Mampaso, A.
Referencia bibliográfica
Revista Mexicana de Astronomia y Astrofisica, 14, 515
Fecha de publicación:
5
1987
Número de citas
0
Número de citas referidas
0
Descripción
New optical and infrared spectroscopic and photometric observations of
the cometary nebula 1548C27 have shown that a young star loosing mass at
high velocity (hundreds of km 1) is the source of energy of the nebula.
This source is suggested from its infrared luminosity, to be a Herbig
Ae-Be type star surrounded by a dusty envelope radiating at a range of
temperatures (60-900 K