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Molecular gas in galaxies: changing conditions from disks to starbursts

Part of: IAU Issue 315 - From Interstellar Clouds...

Published online by Cambridge University Press:  12 September 2016

Christine D. Wilson
Christine D. Wilson*
Affiliation:
Department of Physics and Astronomy, McMaster University, Hamilton, Ontario, CanadaL8S 4M1 email: [email protected]
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Abstract

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In understanding galaxy evolution, one central question is how star formation is regulated in galaxies. Changes in star formation rates are likely tied to changes in the interstellar medium, particularly the molecular gas which is the fuel for star formation. I will discuss our recent results which use data from the Herschel Space Observatory, the Atacama Large Millimeter/submillimeter Array, and other telescopes to determine the typical density, temperature, and surface density of the molecular gas in various nearby galaxies. Comparing the properties of molecular gas in starburst and other active galaxies with more quiescent spiral disks provides some clues as to how changes in the physical state of the gas, such as mean density, can lead to enhanced star formation rates.

Keywords

ISM: moleculesgalaxies: spiralgalaxies: starburst
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S315: From Interstellar Clouds to Star-Forming Galaxies: Universal Processes? , August 2015 , pp. 199 - 206
Copyright
Copyright © International Astronomical Union 2016 

References

Bigiel, F., Leroy, A. K., Walter, F., et al. 2011, AJ, 730, L13 Google Scholar
Boselli, A., Cortese, L., Boquien, M., Boissier, S., Catinella, B., Lagos, C., & Saintonge, A. 2014, A&A, 564, A66 Google Scholar
Cortese, L., Ciesla, L., Boselli, A., et al. 2012, A&A, 540, A52 Google Scholar
Draine, B. T. & Li, A. 2007, ApJ, 657, 810 CrossRefGoogle Scholar
Fumagalli, M. & Gavazzi, G. 2008, A&A, 490, 571 Google Scholar
Haynes, M. P., Giovanelli, R., & Chincarini, G. L. 1984, ARAA, 22, 445 Google Scholar
Helfer, T. T. & Blitz, L. 1993 ApJ, 419, 86 Google Scholar
Hollenbach, D., Kaufman, M. J., Neufeld, D., Wolvire, M., & Goicoechea, J. R. 2012, ApJ, 754, 105 Google Scholar
Huang, M.-L. & Kauffmann, G. 2014, MNRAS, 443, 1329 Google Scholar
Kamenetzky, J., Glenn, J., Maloney, P. R. et al. 2011, ApJ, 731, 83 Google Scholar
Kamenetzky, J., Glenn, J., Rangwala, N. et al. 2012, ApJ, 753, 70 Google Scholar
Kannappan, S. J., Stark, D. V., Eckert, K. D., et al. 2013, ApJ, 777, 42 CrossRefGoogle Scholar
Kaufman, M. J., Wolfire, M. G., Hollenback, D. J., & Luhmn, M. L. 1999, ApJ, 527, 795 Google Scholar
Kenney, J. D. P. & Young, J. S. 1989, ApJ, 334, 171 Google Scholar
Koopmann, R. A., Haynes, M. P., & Catinella, B. 2006, AJ, 131, 716 Google Scholar
Mentuch Cooper, E., Wilson, C. D., Foyle, K. et al. 2012, ApJ, 755, 165 Google Scholar
Mok, A., Wilson, C. D., Golding, J. et al. 2016, MNRAS, submittedGoogle Scholar
Parkin, T. J., Wilson, C. D., Schirm, M. R. P., et al. 2013, ApJ, 776, 65 Google Scholar
Pety, J., Schinnerer, E., Leroy, A. K. et al. 2013, ApJ, 779, 43 Google Scholar
Rangwala, N., Maloney, P. R., Glenn, J. et al. 2011, ApJ, 743, 94 Google Scholar
Rangwala, N., Maloney, P., Wilson, C. D., Glenn, J., Kamenetzky, J., & Spinoglio, L. 2015, ApJ, 806, 17 CrossRefGoogle Scholar
Saintonge, A., Kauffmann, G., Wang, J., et al. 2011, MNRAS, 415, 61 Google Scholar
Sandstrom, K. M., Leroy, A. K., Walter, F., et al. 2013, ApJ, 777, 5 Google Scholar
Schinnerer, E., Meidt, S. E., Pety, J. et al. 2013, ApJ, 779, 42 CrossRefGoogle Scholar
Schirm, M. R. P., Parkin, T. J., Wilson, C. D., et al. 2014, ApJ, 781, 101 CrossRefGoogle Scholar
Schirm, M. R. P. 2015, Ph.D. thesis, McMaster UniversityGoogle Scholar
Schirm, M. R. P., Wilson, C. D., Madden, S. C., & Clemens, D. L. 2016, ApJ, submittedGoogle Scholar
Scoville, N., Sheth, K., Walter, F., et al. 2015, ApJ, 800, 70 Google Scholar
Sliwa, K., Wilson, C. D., Petitpas, G. R. et al. 2012, ApJ, 753, 46 Google Scholar
Sliwa, K., Wilson, C. D., Krips, M. et al. 2013, ApJ, 796, L15 Google Scholar
Sliwa, K., Wilson, C. D., Iono, D., Peck, A., & Matsushita, S. 2014, ApJ, 753, 46 Google Scholar
Sliwa, K. 2015, Ph.D. thesis, McMaster UniversityGoogle Scholar
Solanes, J. M., Manrique, A., García-Gómez, C., González-Casado, G., Giovanelli, R., & Haynes, M. P. 2001, ApJ, 548, 97 Google Scholar
Sturm, E., González-Alfonso, E., Veilleux, S., et al. 2011, ApJ, 733, L16 Google Scholar
Tacconi, L., Neri, R., Genzel, R., et al. 2013, ApJ, 768, 74 Google Scholar
Usero, A., Leroy, A. K., Walter, F., et al. 2015, AJ, 150, 115 Google Scholar
van der Tak, F. F. S., Black, J. H., Schier, F. L., Jansen, D. J., & van Dishoeck, E. F. 2007, A&A, 468, 627 Google Scholar
Vlahakis, C., van der Werf, P., Israel, F. P., & Tilanus, R. P. J. 2013, MNRAS, 433, 1837 Google Scholar
Whitmore, B. C., Zhang, Q., Leitherer, C., Fall, S. M., Schweizer, F., & Miller, B. W. 1999, AJ, 118, 1551 Google Scholar
Wilson, C. D., Scoville, N., Madden, S. C., & Charmandaris, V. 2003, ApJ, 599, 1049 Google Scholar
Wilson, C. D., Petitpas, G. R., Iono, D. et al. 2008, ApJS, 178, 189 Google Scholar
Wilson, C. D., Warren, B. E., Israel, F., et al. 2012, MNRAS, 424, 3050 Google Scholar
Wilson, C. D., Rangwala, N., Glenn, J., Maloney, P., Spinoglio, L., & Pereira-Ssantaella, M. 2014, ApJ, 789, L36 Google Scholar