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Molecular gas, stars, and dust in sub-L star-forming galaxies at z ~ 2: Evidence for universal star formation and non-universal dust-to-gas ratio

Published online by Cambridge University Press:  12 September 2016

Miroslava Dessauges-Zavadsky
Affiliation:
Observatoire de Genève, Université de Genève, 51 Chemin des Maillettes, 1290 Versoix, Switzerland
Michel Zamojski
Affiliation:
Observatoire de Genève, Université de Genève, 51 Chemin des Maillettes, 1290 Versoix, Switzerland
Daniel Schaerer
Affiliation:
Observatoire de Genève, Université de Genève, 51 Chemin des Maillettes, 1290 Versoix, Switzerland
Françoise Combes
Affiliation:
Observatoire de Paris, LERMA, 61 Avenue de l'Observatoire, 75014 Paris, France
Eiichi Egami
Affiliation:
Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, United States
Panos Sklias
Affiliation:
Observatoire de Genève, Université de Genève, 51 Chemin des Maillettes, 1290 Versoix, Switzerland
Mark A. Swinbank
Affiliation:
Institute for Computational Cosmology, Durham University, South Road, Durham DH1 3LE, United Kingdom
Johan Richard
Affiliation:
CRAL, Observatoire de Lyon, Université Lyon 1, 9 Avenue Ch. André, 69561 Saint Genis Laval Cedex, France
Tim Rawle
Affiliation:
ESAC, ESA, PO Box 78, Villanueva de la Canada, 28691 Madrid, Spain
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Abstract

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Current star-forming galaxies (SFGs) with CO measurements at z ~ 2 suffer from a bias toward high star formation rates (SFR) and high stellar masses (M*). It is yet essential to extend the CO measurements to the more numerous z ~ 2 SFGs with LIR < L = 4× 1011 L and M* < 2.5× 1010 M. We have achieved CO, stars, and dust measurements in 8 such sub-L SFGs with the help of gravitational lensing. Combined with CO-detected galaxies from the literature, we find that the LIR, LCO(1−0) data are best-fitted with a single relation that favours a universal star formation. This picture emerges because of the enlarged star formation efficiency spread of the current z>1 SFGs sample. We show that this spread is mostly triggered by the combination of redshift, specific SFR, and M*. Finally, we find evidence for a non-universal dust-to-gas ratio (DGR) with a clear trend for a lower DGR mean in z>1 SFGs by a factor of 2 with respect to local galaxies and high-redshift sub-mm galaxies at fixed about solar metallicity.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2016 

References

Bothwell, M. S., Wagg, J., Cicone, C., et al. 2014, MNRAS, 445, 2599 CrossRefGoogle Scholar
Daddi, E., Dickinson, M., Morrison, G., et al. 2007, ApJ, 670, 156 CrossRefGoogle Scholar
Daddi, E., Bournaud, F., Walter, F., et al. 2010, ApJ, 713, 686 Google Scholar
Dessauges-Zavadsky, M., Zamojski, M., Schaerer, D., et al. 2015, A&A, 577, 50 Google Scholar
Egami, E., Rex, M., Rawle, T. D., et al. 2010, A&A, 518, 12 Google Scholar
Elbaz, D., Dickinson, M., Hwang, H. S., et al. 2011, A&A, 533, 119 Google Scholar
Genzel, R., Tacconi, L. J., Gracia-Carpio, J., et al. 2010, MNRAS, 407, 2091 Google Scholar
Gruppioni, C., Pozzi, F., Rodighiero, G., et al. 2013, MNRAS, 432, 23 CrossRefGoogle Scholar
Magdis, G. E., Daddi, E., Béthermin, M., et al. 2012, ApJ, 760, 6 Google Scholar
Rodighiero, G., Daddi, E., Baronchelli, I., et al. 2011, ApJL, 739, L40 Google Scholar
Saintonge, A., Kauffmann, G., Wang, J., et al. 2011, MNRAS, 415, 61 Google Scholar
Saintonge, A., Lutz, D., Genzel, R., et al. 2013, ApJ, 778, 2 Google Scholar
Sargent, M. T., Daddi, E., Béthermin, M., et al. 2014, ApJ, 793, 19 Google Scholar
Scoville, N., Aussel, H., Sheth, K., et al. 2014, ApJ, 783, 84 Google Scholar
Sklias, P., Zamojski, M., Schaerer, D., et al. 2014, A&A, 561, 149 Google Scholar
Tacconi, L. J., Neri, R., Genzel, R., et al. 2013, ApJ, 768, 74 CrossRefGoogle Scholar