Issue |
A&A
Volume 365, Number 2, January 2001
|
|
---|---|---|
Page(s) | 1 - 10 | |
Section | Cosmology (including clusters of galaxies) | |
DOI | https://doi.org/10.1051/0004-6361:20000002 | |
Published online | 15 January 2001 |
H i observations of giant low surface brightness galaxies *,**
1
National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903, USA
2
Unité Scientifique Nançay, USR CNRS B704, Observatoire de Paris, 5 place Jules Janssen, 92195 Meudon, France
3
DAEC, UMR CNRS 8631, Observatoire de Paris, 5 place Jules Janssen, 92195 Meudon, France
Corresponding author: L. D. Matthews, lmatthew@nrao.edu
Received:
12
July
2000
Accepted:
22
September
2000
We have used the Nançay Radio Telescope to obtain new global H i data
for 16 giant low surface brightness (LSB) galaxies.
Our targets have optical luminosities and disk scale lengths at the
high end for spiral galaxies (
and
kpc for
km s-1 Mpc-1),
but they have diffuse stellar disks, with mean
disk surface brightnesses
magnitude
fainter than normal giant spirals. Thirteen of the galaxies
previously had been detected in H i by other workers,
but the published H i observations were either confused,
resolved by the telescope beam, of low signal-to-noise, or
showed significant discrepancies between
different authors. For the other 3 galaxies, no H i data
were previously available. Several of the galaxies were resolved by the Nançay #1' . #2 E-W beam, so global parameters were derived from
multiple-point mapping observations. Typical H i masses for
our sample are
, with
(in
solar units). All of the observed galaxies have
published optical surface photometry, and we have compiled key optical
measurements for these objects from the literature.
We frequently find significant variations among
physical parameters of giant LSB galaxies reported by
various workers.
Key words: galaxies: distances and redshifts - galaxies: general - galaxies: ISM - radio lines: galaxies
© ESO, 2001
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