Spectrosocpy of NGC 7009 (Phillips+, 2010)

Details Spectrosocpy of NGC 7009 (Phillips+, 2010) Spectrosocpy of NGC 7009 (Phillips+, 2010)

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..74090881p&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/409/881. Originally published in: 2010MNRAS.409..881P

Astronomy and Astrophysics

Astronomy

Planetary Nebulae, Spectroscopy

Scientific paper

NGC 7009 is a fascinating example of a high-excitation, elliptical planetary nebula (PN) containing circumnebular rings, and FLIERs and jets along the major axis. We present visual spectroscopy along multiple position angles through the nucleus, taken with the Observatorio Astronomico Nacional (Mexico); mid-infrared (MIR) spectroscopy and imaging acquired using the Infrared Space Observatory (ISO) and Spitzer Space Telescope (SST), and narrow-band imaging obtained using the Hubble Space Telescope (HST).
(1 data file).

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