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Дата изменения: Tue Nov 24 21:18:57 1998 Дата индексирования: Sat Sep 11 22:07:47 2010 Кодировка: Поисковые слова: solar eclipse |
and@sao.ru
A.V. Ugryumov1 - D. Engels2 -
V.A. Lipovetsky1
- H.-J. Hagen2 - U. Hopp38
- S.A. Pustilnik1 - A.Yu. Kniazev1 - G. Richter
4
- Yu.I. Izotov5 - C.C. Popescu67
Special Astrophysical Observatory, Nizhnij Arkhyz, Karachai-Circessia, 357147, Russia - Hamburger Sternwarte, Gojenbergswerg 112, D-21029 Hamburg, Germany - Universitäts-Sternwarte, Scheiner Str. 1, D-81679, München, Germany - Astrophysikalisches Institut Potsdam, An der Sternwarte 16, D-14482 Potsdam, Germany - Main Astronomical Observatory, Goloseevo, Kiev-22, 252650, Ukraine - Max-Planck Institut für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany - The Astronomical Institute of the Romanian Academy, Str. Cutitul de Argint 5, 75212 Bucharest, Romania - Visiting astronomer at Calar Alto Observatory, Spain
Received ; Accepted
We present first results of
the Hamburg/SAO Survey for Emission-Line Galaxies (HSS therein, SAO -
Special Astrophysical Observatory, Russia) which is based on the digitized
objective-prism photoplates database of the Hamburg Quasar Survey (HQS).
The main goal of this survey is the search for emission-line galaxies (ELG)
in order to create a new deep sample of blue compact galaxies (BCG) in
a large sky area. Another important goal of this work is to search for new
extremely low-metallicity galaxies.
We present the first results of spectroscopy obtained with the 2.2m
telescope at the German-Spanish Observatory at Calar Alto, and with the 6m
telescope at the Russian Special Astrophysical Observatory. The primary ELG
candidate selection criteria applied were a blue continuum (near
4000 Å) and the presence of emission lines close to
5000 Å recognized on digitized prism spectra of galaxies with
magnitudes in the range B =
.
The spectroscopy resulted
in the detection or/and quantitative spectral classification of 74
emission-line objects. Of them 55 are newly discovered,
and 19 were already known as galaxies before. 11 of the latter have
redshifts and are known ELGs. For most of the known galaxies emission
line ratios were measured for the first time and an improved classification
is presented.
47 objects are classified as BCGs, one as Sy2 galaxy, six as
probable LINERs, and four as new QSOs. The remaining galaxies do not show
significant H
and [O III]
4959,5007 Å emission lines, and are likely either low-ionization starburst or dwarf
amorphous nuclear starburst galaxies.
surveys - galaxies: fundamental parameters - galaxies: distances and redshifts - galaxies: starburst - galaxies: compact