Emission-line stars and PNe in the SMC (Meyssonnier+ 1993)

Details Emission-line stars and PNe in the SMC (Meyssonnier+ 1993) Emission-line stars and PNe in the SMC (Meyssonnier+ 1993)

Sep 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ycat..41020451m&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/102/451. Originally published in: 1993A&AS..102..451M

Computer Science

Magellanic Clouds, Stars: Emission, Planetary Nebulae

Scientific paper

An objective-prism survey of the Small Magellanic Cloud (SMC) has been performed through an H-α + [NII] interference filter, using the 90cm Curtis Schmidt telescope of Cerro Tololo. 1898 emission-line objects have been detected in the main body of this galaxy, almost quadrupling the number of those found in the same region by the previous objective-prism surveys. Among these objects are newly discovered planetary nebulae, compact HII regions and late-type stars. Continuum intensity, as well as the shape and relative strength of the H-α emission-line have been estimated; coordinates, cross-identifications for the listed objects are provided. The original paper contains in addition finding charts. (2 data files).

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