Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-10-25
Astronomy and Astrophysics
Astrophysics
4 pages, Latex file, 2 Postscript Figures, aa.cls and psfig.sty stylefiles included. Accepted to Astronomy and Astrophysics Le
Scientific paper
The (J,K) = (1,1), (2,2), (3,3), and (4,4) inversion lines of ammonia (NH3) have been detected toward the nuclear 40'' sized bar of the nearby spiral galaxy Maffei 2. The relative intensities of the ammonia lines are characterized by a rotational temperature of 85 K. This is higher than rotational temperatures measured toward IC342 and most Galactic Center clouds, implying kinetic temperatures of at least 100 K. Since the kinetic temperature of the gas is larger than that of the dust, NH3 is tracing a particularly dense warm gas component that is heated by young massive stars, cloud-cloud collisions, or ion-slip heating in the nuclear starburst. The gas north of the nucleus (V(LSR} = -80 km/s) is more highly excited than the gas further south (+6 km/s). This asymmetry might be related to a pronounced morphological distortion that is observed in the north-eastern part of the galaxy.
Falcke Heino
Hagiwara Yoshiaki
Henkel Carsten
Mauersberger Rainer
Peck Alison Beth
No associations
LandOfFree
Dense Gas in Nearby Galaxies: XIV. Detection of hot ammonia in Maffei 2 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Dense Gas in Nearby Galaxies: XIV. Detection of hot ammonia in Maffei 2, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dense Gas in Nearby Galaxies: XIV. Detection of hot ammonia in Maffei 2 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-105203