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Дата изменения: Tue Feb 8 09:57:26 2000 Дата индексирования: Sat Sep 11 20:38:18 2010 Кодировка: |
Thirteen non emission-line objects are hard to classify at all. Their
continua have too low signal-to-noise ratio to detect trustworthy
absorption features, or the EW of the emission lines is too small. Six
of them are certainly non-stellar on DSS images, and classified as
well as non-stellar in the APM database. From our spectra in the range
4000 to
7300-8000 Å, we can exclude the
presence of strong H
.
The remaining 7 objects are
indistinguishable from stellar ones, and we suggest that most of them
are galactic stars. One of the galaxies - namely HS 1232+3609, was
presented after our observations in the paper by Popescu et al.
([1998]) as ELG with z=0.2529. Our spectrum is too noisy,
and we could not identify any significant emission with this redshift.