/ftp/cats/aliases/K/./KW_1_



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J/AN/324/437  New Ha emission stars towards Gal Bulge   (Kohoutek+, 2003)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table1.dat table1a.dat table2.dat notes.dat table3.dat table3a.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/AN/324/437
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drwxr-xr-x 4 cats root 60 Jan 29 2012 [Up] drwxr-xr-x 2 cats root 4096 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 519 Dec 19 2022 .message -rw-r--r-- 1 cats archive 6519 Nov 28 2007 ReadMe -rw-r--r-- 1 cats archive 314 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2352 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 2788 Jul 16 2005 notes.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 5194 Jul 15 2005 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 477 Jul 15 2005 table1a.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 1293 Jul 15 2005 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 2869 Jul 15 2005 table3.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 277 Jul 15 2005 table3a.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/AN/324/437 Halpha emission stars toward Bulge (Kohoutek+, 2003) ================================================================================ New H-alpha emission stars towards the Galactic Bulge. Kohoutek L., Wehmeyer R. <Astron. Nachr., 324, 437-444 (2003)> =2003AN....324..437K ================================================================================ ADC_Keywords: Stars, emission ; Spectroscopy Keywords: Galaxy: center - surveys - stars: emission-line Abstract: This paper is dealing with the investigation of H-alpha emission stars towards the galactic bulge. In this important region 533 H-alpha emission stars have already been discovered. We add 98 new and 9 possible new (perhaps identical with known objects) H-alpha emission stars found in the objective-prism survey of planetary nebulae and we give the identification charts, the accurate coordinates as well as a rough description. The distribution in l, b of all objects shows the expected concentration towards the galactic equator with the maximum near l=0 and b=0 distorted probably due to strong interstellar extinction.