/ftp/cats/A+AS/102/451



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J/A+AS/102/451    Emission-line stars and PNe in the SMC    (Meyssonnier+ 1993)
The following files can be converted to FITS (extension .fit or fit.gz)
	table2.dat notes.dat table2x.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+AS/102/451
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drwxr-xr-x 18 cats archive 303 Dec 12 2012 [Up] drwxr-xr-x 4 cats archive 4096 Jun 29 2023 [TAR file] -rw-r--r-- 1 cats archive 490 Dec 19 2022 .message -r--r--r-- 1 cats archive 11288 Dec 12 2012 ReadMe -rw-r--r-- 1 cats archive 1010 Dec 12 2012 +footg5.gif -rw-r--r-- 1 cats archive 2577 Dec 12 2012 +footg8.gif -r--r--r-- 1 cats archive 8200 Sep 20 1996 notes.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 98611 Jun 26 1993 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 95679 Dec 12 2012 table2x.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+AS/102/451 Emission-line stars and PNe in the SMC (Meyssonnier+ 1993) ================================================================================ A new catalogue of H-alpha emission-line stars and small nebulae in the Small Magellanic Cloud Meyssonnier N., Azzopardi M. <Astron. Astrophys. Suppl. Ser. 102, 451 (1993)> =1993A&AS..102..451M ================================================================================ ADC_Keywords: Magellanic Clouds ; Stars, emission ; Planetary nebulae Keywords: galaxies: Magellanic Clouds - stars: emission-line - H II regions - planetary nebulae : general - surveys - catalogs Description: An objective-prism survey of the Small Magellanic Cloud (SMC) has been performed through an H-alpha + [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-alpha emission-line have been estimated; coordinates, cross-identifications for the listed objects are provided. The original paper contains in addition finding charts.