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

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

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15...82r&link_type=abstract

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J.

Astronomy and Astrophysics

Astronomy

1

Planetary Nebula, Ism: Jets And Outflows

Scientific paper

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).

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