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5.4. New high-resolution observations of molecular gas towards the center of spiral galaxies

Observations and numerical simulations

Published online by Cambridge University Press:  25 May 2016

S. Garcia-Burillo
S. Garcia-Burillo*
Affiliation:
Observatorio Astronómico Nacional, Campus Universitario, Apdo 1143, 28800 Alcalá de Henares, SPAIN

Extract

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We discuss the major results from a study of the molecular gas distribution and dynamics in the nuclear disks (ND) of a limited sample of nearby spirals: NGC891, NGC5907, NGC4565, NGC4013, NGC4321, M82, NGC3626 and NGC3593. The main objective is to search for observational evidences of secular evolution along the Hubble sequence in spirals and to study the specific role of bars in the process.

Type
Part II. Nuclear Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 184: The Central Regions of the Galaxy and Galaxies , 1998 , pp. 217 - 218
Copyright
Copyright © Kluwer 1998 

References

García–Burillo, S., Guélin, M., 1995, A&A, 299, 657.Google Scholar
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Gómez de Castro, A.I., García–Burillo, S., 1997, A&A, 322, 381.Google Scholar
García–Burillo, S., Sempere, M.J., Combes, F., Neri, R., 1997, A&A, submitted.Google Scholar