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Evidence for Shocks and Increased SFE in the Lyman Alpha Reference Sample

Published online by Cambridge University Press:  09 February 2015

Johannes Puschnig ,
Matthew Hayes  and
Göran Östlin
Johannes Puschnig
Affiliation:
Department of Astronomy, Oskar Klein Centre, Stockholm University email: [email protected]
Matthew Hayes
Affiliation:
Department of Astronomy, Oskar Klein Centre, Stockholm University email: [email protected]
Göran Östlin
Affiliation:
Department of Astronomy, Oskar Klein Centre, Stockholm University email: [email protected]
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We report on first molecular gas observations in the Lyman Alpha Reference Sample (LARS; Hayes et al.2013, 2014, Östlin et al.2014), which were performed using the 45m telescope at the Nobeyama Radio Observatory (NRO). The beamsize at the observed 12CO (1–0) emission is ≈ 15” corresponding to ≈ 12kpc at the given redshift of z ≈ 0.04. We detected strong 12CO emission in LARS 3 (Arp 238), marginally detected LARS 8 (SDSS 1250+0734) and derived an upper limit for LARS 9 (IRAS 08208+2816).

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S309: Galaxies in 3D across the Universe , July 2014 , pp. 335 - 336
Copyright
Copyright © International Astronomical Union 2015 

References

Hayes, M., Östlin, Duval, F., et al. 2014, ApJ, 782, 6Google Scholar
Magdis, G. E., Daddi, E., Elbaz, D., et al. 2011, ApJ, 740, 15CrossRefGoogle Scholar
Zubovas, K., Sabulis, K., Naujalis, R. 2014 MNRAS, 442, 2837Google Scholar
Hayes, M., Östlin, G., Schaerer, D., et al. 2013, ApJL, 765, L27Google Scholar
Östlin, G., Hayes, M., Duval, F., et al. 2014, ApJ, in prep.Google Scholar