Spectra of blue compact galaxies (Kong+, 2002)

Details Spectra of blue compact galaxies (Kong+, 2002) Spectra of blue compact galaxies (Kong+, 2002)

Aug 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ycat..33960503k&link_type=abstract

VizieR On-line Data Catalog: J/A+A/396/503. Originally published in: 2002A&A...396..503K

Astronomy and Astrophysics

Astronomy

Galaxies: Spectra

Scientific paper

This is the second paper in a series studying the star formation rates, stellar components, metallicities, and star formation histories and evolution of a sample of blue compact galaxies. We analyzed spectral properties of 97 blue compact galaxies, obtained with the Beijing Astronomical Observatory (China) 2.16m telescope, with spectral range 3580{AA}-7400{AA}.
We classify the spectra according to their emission lines: 13 of the total 97 BCG sample are non-emission line galaxies (non-ELGs); 10 have AGN-like emission (AGNs), and 74 of them are star-forming galaxies (SFGs). Emission line fluxes and equivalent widths, continuum fluxes, the 4000A Balmer break index and equivalent widths of absorption lines are measured from the spectra. Please find more detail information in http://optik2.mtk.nao.ac.jp/~xkong/bcg/
(5 data files).

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