We present the results of a survey for CO line emission from a sample of nearby QSO hosts taken from the Hamburg/ESO survey (HES) and the Ve Β΄ron-Cetty and Ve Β΄ron quasar catalogue. From a total of 39 observed sources we clearly detected five objects with >10r signals (
β¦ LIBER β¦
Molecular Gas in Galaxies
β Scribed by Francoise Combes
- Book ID
- 110316316
- Publisher
- Springer Netherlands
- Year
- 2001
- Tongue
- English
- Weight
- 85 KB
- Volume
- 277
- Category
- Article
- ISSN
- 0004-640X
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
Molecular gas in QSO host galaxies
β
T. Bertram; A. Eckart; M. Krips; C. Straubmeier; S. Fischer; J.G. Staguhn
π
Article
π
2006
π
Elsevier Science
π
English
β 218 KB
Molecular and Ionized Gas in Galaxies
β
L. G. Hou
π
Article
π
2013
π
University of Chicago Press
π
English
β 307 KB
Molecular gas in blue compact dwarf gala
β
L. T. Barone; A. Heithausen; S. HΓΌttemeister; T. Fritz; U. Klein
π
Article
π
2000
π
John Wiley and Sons
π
English
β 322 KB
Molecular gas in intermediate-redshift u
β
R. Braun; A. Popping; K. Brooks; F. Combes
π
Article
π
2011
π
John Wiley and Sons
π
English
β 657 KB
Molecular gas properties in interacting
β
Susanne Aalto
π
Article
π
2007
π
Elsevier Science
π
English
β 444 KB
Molecular line emission is a useful tool for probing the highly obscured inner kpc of starburst galaxies -and of galaxies that harbour an enshrouded active nucleus. Molecular line ratios will serve as diagnostic tools of the physical conditions of the gas -but also of its chemical properties. Both p
Interferometer observations of molecular
β
S. GarcΓa-Burillo; F. Combes; A. Usero; A. Fuente
π
Article
π
2009
π
John Wiley and Sons
π
English
β 200 KB