Comparison of photometric parameters of LSB and HSB edge-on galaxies.pdf
文本预览下载声明
a
r
X
i
v
:
a
s
t
r
o
-
p
h
/
0
0
0
7
2
4
2
v
1
1
7
J
u
l
2
0
0
0
The paper was presented as a poster
at JENAM-2000 meeting
(29 May - 3 June, Moscow, Russia)
Comparison of photometric parameters
of LSB and HSB edge-on galaxies.
Bizyaev D.V.
dmbiz@sai.msu.ru
Sternberg Astronomical Institute, Moscow, Russia
Abstract
Photometric parameters of stellar disks and bulges for several edge-on galaxies from
the Catalog of Flat Galaxies (FGC) were determined. We discuss a difference between
photometric parameters of LSB and HSB galaxies from our sample.
Also we present results of R CCD photometry of edge-on galaxy RFGC 3647. Depro-
jecting this galaxy we show that it has thin LSB disk (central surface brightness 22m.2
in R) and high ratio of radial to vertical scale lengths. It is shown that initially gaseous
disk of the galaxy was unstable and its velocity dispersion was low. Stellar disk of this
LSB galaxy was not heated significantly since that time.
1
Introduction
The main properties of LSB galaxies are low surface and volume density of stellar disks,
low metallicity and star formation rates and they are more extended than ”normal”,
HSB galaxies (see de Block etc., 1996, Bothun etc. 1997, Pickering etc.1994). The
existence of LSB galaxies observed edge-on have remarked in papers of Karachentsev etc.
(1992), in description of Flat Galaxies Catalog (Karachentsev etc., 1993). In works of
Reshetnikov and Combes (1996, 1997, hereafter RC96, RC97) small sample of unwarped
edge-on galaxies was investigated and some galaxies of the sample were suspected to be
LSB galaxies.
There was no studies of vertical structure of a sample LSB galaxies as well as a
comparison of photometric parameters of LSB and HSB spirals obtained from observations
of edge-on objects. We are using the sample of unperturbed galaxies from papers RC96
and RC97 for these purposes.
The sample of the galaxies.
Images of seven edge-on galaxies obtained in I (Causins) passband were taken at OHP
observatory (Fra
显示全部