Aperture Synthesis CO and HCN Observationsof M51: Dense Molecular Disk around a Low-Luminosity Active Galactic Nucleus

Details Aperture Synthesis CO and HCN Observationsof M51: Dense Molecular Disk around a Low-Luminosity Active Galactic Nucleus Aperture Synthesis CO and HCN Observationsof M51: Dense Molecular Disk around a Low-Luminosity Active Galactic Nucleus

Apr 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apj...461l..29k&link_type=abstract

Astrophysical Journal Letters v.461, p.L29

Astronomy and Astrophysics

Astronomy

58

Galaxies: Individual Messier Number: M51, Galaxies: Ism, Galaxies: Nuclei, Galaxies: Seyfert

Scientific paper

We performed aperture synthesis CO (J = 1 --> 0) and HCN (J = 1 --> 0) observations of M51 using the Nobeyama Millimeter Array with spatial resolutions of 4" (corresponding to 190 pc at D = 9.6 Mpc) and 6", respectively. Higher resolution (4") HCN images were also made to resolve the structure of the circumnuclear region. The CO map shows clumpy structures that are mainly distributed along a pair of inner spiral arms. In contrast, intense HCN emission was detected in the central region (r < 200 pc) where CO emission is depressed. The obtained 4" resolution HCN maps suggest the existence of a rotating dense molecular disk (the nuclear disk) whose rotation axis (P.A. ~ 160 deg) is just aligned to the direction of the nuclear jet (P.A. ~ 165 deg), not to the rotation axis of the galactic plane. The radius of the nuclear disk is estimated to be 70 pc, and the rotation velocity of the nuclear disk is 16(sin i)-1 km s-1 at r = 70 pc, where i is the inclination angle of the nuclear disk. The HCN/CO integrated intensity ratio exceeds 0.3 inside r = 140 pc, which is a factor of 10 larger than those of the spiral arm region (r > 300 pc). The high HCN/CO ratio means that most of the molecular gas is dense enough to excite HCN (J = 1 --> 0) emission (n_{{H}2} ~ 105 {cm}^{-3}) . The column density of molecular hydrogen toward the nucleus was estimated to be N_{{H}2} > 1.5 x 1023 {cm}^{-2} , which plausibly accounts for the large amount of material absorbing X-rays from the nucleus. These results suggest that the 50--100 pc scale molecular disk would play an important role for the obscuration of a weak Seyfert nucleus in M51.

Affiliated with

Also associated with

No associations

Rating

Aperture Synthesis CO and HCN Observationsof M51: Dense Molecular Disk around a Low-Luminosity Active Galactic Nucleus 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 Aperture Synthesis CO and HCN Observationsof M51: Dense Molecular Disk around a Low-Luminosity Active Galactic Nucleus, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Aperture Synthesis CO and HCN Observationsof M51: Dense Molecular Disk around a Low-Luminosity Active Galactic Nucleus will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1334933