Issue |
Astron. Astrophys. Suppl. Ser.
Volume 136, Number 1, April I 1999
|
|
---|---|---|
Page(s) | 179 - 187 | |
DOI | https://doi.org/10.1051/aas:1999459 | |
Published online | 15 April 1999 |
Spectroscopic observations of southern nearby galaxies*
I. NGC 2442
1
Instituto Argentino de Radioastronomía, C.C. 5, 1894 Villa Elisa, Prov. de Bs.As., Argentina
2
Observatorio Astronómico de Córdoba, Laprida 854, 5000 Córdoba, Argentina
Send offprint request to: E. Bajaja
Received:
31
August
1998
Accepted:
4
January
1999
The galaxy NGC 2442 was observed with a REOSC spectrograph,
installed in the 2.15 m CASLEO telescope, in order to derive galactic
parameters from the observed optical lines and to compare them with
the results of radioastronomical observations made in the continuum,
at 843 MHz, with the MOST and in the CO lines with the SEST telescope.
Recent publications allowed us to extend the comparison to results from
interferometric observations of Hα and Hi 21 cm lines
and of the continuum at 1415 MHz.
The long slit observations were made placing the 58 slit at six
different positions on the optical image of the galaxy. The emission
line intensity ratios at the nuclear region indicate that NGC 2442
is a LINER. The electron temperature and volume density are
14 000 K and
530
cm-3, respectively. In contrast, a spectrum of a region
87″ to the NE shows the typical characteristics of a Hii
region.
In this case
6 500 K and
10 cm-3. Good correlations
between the distributions of intensities, velocity fields and rotation
curves have been found for the optical and radio lines.
It is shown that the three intensity peaks along the line at PA = 40°
were not resolved by the observations at radio frequencies.
The steep central rotation curve seen in CO has been confirmed and improved
showing the existence of a disc or a ring, with a radius of 12
5,
rotating at 216/sin(i)
. Two velocity components
in three optical spectra obtained in the nuclear region, have been related to
two small Hα regions close to the nucleus and to the central ring.
Asymmetries in the distributions of the emitting sources and
irregularities in their velocity fields indicate the need of modelling the
galaxy before any dynamical study is attempted.
Key words: galaxies: NGC 2442; kinematics and dynamics; nuclei; ISM
© European Southern Observatory (ESO), 1999