Issue |
A&A
Volume 421, Number 2, July II 2004
|
|
---|---|---|
Page(s) | 539 - 554 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361:20035847 | |
Published online | 22 June 2004 |
Deep VLT spectroscopy of the blue compact dwarf galaxies Tol 1214–277 and Tol 65 *,**,***
1
Main Astronomical Observatory, Ukrainian National Academy of Sciences, 27 Zabolotnoho str., Kyiv 03680, Ukraine
2
Universitäts – Sternwarte, Geismarlandstraße 11, 37083 Göttingen, Germany
3
Astronomy Department, University of Virginia, Charlottesville, VA 22903, USA
Corresponding author: Y. I. Izotov, izotov@mao.kiev.ua
Received:
11
December
2003
Accepted:
29
March
2004
We present VLT spectroscopic observations with different
spectral resolutions and different slit orientations of the two
metal-deficient blue compact dwarf (BCD) galaxies Tol 1214–277 and Tol 65.
The oxygen abundances in the brightest H ii regions of Tol 1214–277 and
Tol 65 are found to be and
,
or
/24. The nitrogen-to-oxygen
abundance ratios in the two galaxies are log N/O = –
and
–
and lie in the narrow
range found for other most metal-deficient BCDs.
The helium mass fraction derived in several H ii regions in both
galaxies is consistent with a high primordial helium
mass fraction,
.
We confirm the detection of the high-ionization forbidden emission line
[Fe v] λ4227 in the spectrum of Tol 1214–277.
Additionally, weak [Ne iv] λ4725, [Fe vi] λ5146,
λ5177, and
[Fe vii] λ5721, λ6087 emission lines are detected in
the high-resolution spectrum of Tol 1214–277. The detection of these lines
implies the presence of hard radiation with photon energy in the range
~4–8 Ryd.
Emission lines are detected in the spectra of eight galaxies
in the fields of Tol 1214–277 and Tol 65. Seven of these galaxies are
background objects,
while one galaxy has a redshift close to that of Tol 1214–277.
Situated at a projected distance of ~14.5 kpc from Tol 1214–277, this
galaxy is probably a companion of the BCD.
Key words: galaxies: starburst / galaxies: abundances / galaxies: individual: Tol 1214–277 / galaxies: individual: Tol 65
Based on observations obtained at the European Southern Observatory, Paranal, Chile (ESO Programs 63.P-0003 and 65.N-0642).
© ESO, 2004
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