A new, kinematically anomalous HI component in the spiral galaxy NGC 2403

F Fraternali*, T Oosterloo, R Sancisi, G van Moorsel

*Bijbehorende auteur voor dit werk

OnderzoeksoutputAcademicpeer review

Samenvatting

We discuss new, high-sensitivity H I observations of the spiral galaxy NGC 2403, which show extended emission at anomalous velocities with respect to the "cold" disk. This "anomalous" gas component (similar to1/10 of the total H I mass) is probably located in the region of the halo and rotates more slowly (similar to 20-50 km s(-1)) than the gas in the disk. Moreover, it shows a distortion in the velocity field that we interpret as a large-scale radial motion (10-20 km s(-1) inflow) toward the center of the galaxy. The most likely explanation for its origin and kinematics seems to be that of a galactic fountain. There is, however, a significant part of the anomalous gas that seems to be moving contrary to rotation and is difficult to understand in such a picture. These anomalous gas complexes discovered in NGC 2403 may be analogous to the high-velocity clouds of our Galaxy. They may be rather common in spiral galaxies and not have been detected yet for lack of sensitivity.

Originele taal-2English
Pagina's (van-tot)L47-L50
Aantal pagina's4
TijdschriftAstrophysical Journal
Volume562
Nummer van het tijdschrift1
StatusPublished - 20-nov-2001

Citeer dit