Observations of the Jet-Like Structure Associated with the Binary Planetary Nebula GLMP 621

Bibcode
2003RMxAC..15...82R
Riera, A.; García-Lario, P.; Manchado, A.; Suárez, O.; García-Hernández, D. A.; Guerrero, M. A.
Bibliographical reference

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J. Arthur & W. J. Henney) Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias) Vol. 15, pp. 82-82 (2003) (http://www.astroscu.unam.mx/~rmaa/)

Advertised on:
1
2003
Number of authors
6
IAC number of authors
1
Citations
1
Refereed citations
0
Description
GLMP 621 (IRAS 17395-0841) was first identified as a possible new planetary nebula on the basis of its IRAS colors (García-Lario et al. 1997). A few years ago it was confirmed as such through spectroscopic observations where nebular emission lines corresponding to a prototypical low-excitation planetary nebula were detected superimposed on a strong, red continuum corresponding to a star of intermediate spectral type (García-Lario et al. 1997).
Type
Non-refereed

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