A probable planetary nebula in the direction of the young open cluster NGC 3572

Details A probable planetary nebula in the direction of the young open cluster NGC 3572 A probable planetary nebula in the direction of the young open cluster NGC 3572

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pasp..103..491p&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 103, June 1991, p. 491-493.

Astronomy and Astrophysics

Astronomy

4

Emission Spectra, Galactic Clusters, H Alpha Line, Planetary Nebulae, Galactic Structure, Ring Structures

Scientific paper

The discovery of a ringlike emission feature located along the time of sight toward the young open cluster NGC 3572 is reported. The small feature is prominent in H-alpha but has no central star brighter than magnitude V about 20 and is barely detectable in U, B, and V frames. The appearance of the ring is consistent with it being a PN at an unknown distance.

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