The Molecular Gas Content of Massive Spirals at z = 1.5

Details The Molecular Gas Content of Massive Spirals at z = 1.5 The Molecular Gas Content of Massive Spirals at z = 1.5

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..419..306d&link_type=abstract

Galaxy Evolution: Emerging Insights and Future Challenges ASP Conference Series, Vol. 419, proceedings of a conference held 11-1

Astronomy and Astrophysics

Astronomy

Scientific paper

Following our seminal discovery with IRAM-PdBI of giant molecular gas reservoirs inside two typical, near-IR selected galaxies at z = 1.5 (Daddi et al. 2008), we have now observed a total of six z = 1.5 galaxies in CO[2-1] and detected all of them. Observations of CO[3-2] in one source strikingly revealed the presence of Milky Way like, low-excitation gas. Higher resolution CO[2-1] observations for two galaxies revealed 10 kpc size, galaxy wide gas extension.

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