Spectral survey of Case emission-line galaxies with the 6 M Russian telescope

Details Spectral survey of Case emission-line galaxies with the 6 M Russian telescope Spectral survey of Case emission-line galaxies with the 6 M Russian telescope

Aug 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26as..131..295u&link_type=abstract

Astronomy and Astrophysics Supplement, v.131, p.295-302

Astronomy and Astrophysics

Astrophysics

13

Surveys, Galaxies: Fundamental Parameters, Galaxies: Distances And Redshifts, Galaxies: Starburst, Galaxies: Compact

Scientific paper

The results of the follow-up spectroscopy of 178 emission-line galaxy (ELG) candidates from the Case objective-prism survey and nine Markarian galaxies with the 6 m telescope are described. Only the candidates classified in the Case survey as those with emission lines were observed with the aim to form a statistical sample of blue compact galaxies (BCGs) with strong emission lines in the zone alpha = 8() h /16() h, and delta = +29(deg) /+38(deg) . We present the redshifts, equivalent widths and flux ratios for the strongest lines and the spectrum type for most of the galaxies with detected emission lines. A significant fraction (~ 23%) of the observed Case galaxies do not show emission lines in blue. Preliminary analysis of the data is presented and the properties of the observed ELGs are compared with those of other known samples.
Tables 2 to 4 are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/Abstract.html

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