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Dwarf galaxies at low and high redshift

Published online by Cambridge University Press:  30 October 2019

Xu Kong
Affiliation:
Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Hefei 230026, China email: [email protected] School of Astronomy and Space Science, University of Science and Technology of China, Hefei 230026, China
Jianhui Lian
Affiliation:
Institute of Cosmology and Gravitation, University of Portsmouth, Burnaby Road, Portsmouth PO1 3FX, UK
Yulong Gao
Affiliation:
Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Hefei 230026, China email: [email protected] School of Astronomy and Space Science, University of Science and Technology of China, Hefei 230026, China
Zuyi Chen
Affiliation:
Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Hefei 230026, China email: [email protected] School of Astronomy and Space Science, University of Science and Technology of China, Hefei 230026, China
Guangwen Chen
Affiliation:
Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Hefei 230026, China email: [email protected] School of Astronomy and Space Science, University of Science and Technology of China, Hefei 230026, China
Zesen Lin
Affiliation:
Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Hefei 230026, China email: [email protected] School of Astronomy and Space Science, University of Science and Technology of China, Hefei 230026, China
Haiyang Liu
Affiliation:
Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Hefei 230026, China email: [email protected] School of Astronomy and Space Science, University of Science and Technology of China, Hefei 230026, China
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Abstract

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The overwhelming majority of galaxies in the Universe are dwarf galaxies. But although they are important components in understanding galaxy evolution, these systems are typically too faint to be observed at high redshifts. However, we are able to obtain an unobscured view of early star formation and chemical enrichment in these galaxies at low redshift and low-redshift analogs at high redshift. In this talk, I will review the mass-metallicity relation, the mass-star formation rate relation of galaxies, the classifications of dwarf galaxies, and the importance of dwarf galaxies for both astronomy and physics. Then I will introduce some work in our group on connections among between different types of dwarf galaxies,the mass-metallicity relations and the main sequence relations of dwarf galaxies, using the deep optical and near infrared images and spectra of large dwarf galaxy sample. At the end, I will talk about some projects of dwarf galaxies we are working on, including the spectroscopic survey for compact dwarf galaxies using the LAMOST.

Type
Contributed Papers
Copyright
© International Astronomical Union 2019 

References

Andrews, B. H., & Martini, P. 2013, ApJ, 765, 140 CrossRefGoogle Scholar
Brinchmann, J., Charlot, S., White, S. D. M., et al . 2004, MNRAS, 351, 1151 CrossRefGoogle Scholar
Gao, Y.-L., Lian, J.-H., Kong, X., et al . 2017, RAA, 17, 041 Google Scholar
Heckman, T. M., Hoopes, C. G., Seibert, M., et al . 2005, ApJ(Letters), 619, L35 Google Scholar
Henry, A., Scarlata, C., Domnguez, A., et al . 2013, ApJ(Letters), 776, L27 Google Scholar
Janowiecki, S., & Salzer, J. J. 2014, ApJ, 793, 109 CrossRefGoogle Scholar
Janz, J., Laurikainen, E., Lisker, T., et al . 2014, ApJ, 786, 105 CrossRefGoogle Scholar
Kong, X., & Cheng, F. Z. 2002, A&A, 389, 845 Google Scholar
Kong, X., Fang, G., Arimoto, N., & Wang, M. 2009, ApJ, 702, 1458 CrossRefGoogle Scholar
Lequeux, J., Peimbert, M., Rayo, J. F., Serrano, A., & Torres-Peimbert, S. 1979, A&A, 80, 155 Google Scholar
Lian, J. H., Li, J. R., Yan, W., & Kong, X. 2015, MNRAS, 446, 1449 CrossRefGoogle Scholar
Lian, J. H., Kong, X., Jiang, N., Yan, W., & Gao, Y. L. 2015, MNRAS, 451, 1130 CrossRefGoogle Scholar
Lian, J., Hu, N., Fang, G., Ye, C., & Kong, X. 2016, ApJ, 819, 73 CrossRefGoogle Scholar
Meyer, H. T., Lisker, T., Janz, J., & Papaderos, P. 2014, A&A, 562, A49 Google Scholar
Micheva, G., Östlin, G., Bergvall, N., et al . 2013, MNRAS, 431, 102 CrossRefGoogle Scholar
Maiolino, R., Nagao, T., Grazian, A., et al . 2008, A&A, 488, 463 Google Scholar
Overzier, R. A., Heckman, T. M., Wang, J., et al . 2011, ApJ(Letters), 726, L7 Google Scholar
Pan, Z., Zheng, X., & Kong, X. 2017, ApJ, 834, 39 CrossRefGoogle Scholar
Speagle, J. S., Steinhardt, C. L., Capak, P. L., & Silverman, J. D. 2014, ApJS, 214, 15 CrossRefGoogle Scholar
Tolstoy, E., Hill, V., & Tosi, M. 2009, ARAA, 47, 371 CrossRefGoogle Scholar
Tremonti, C. A., Heckman, T. M., Kauffmann, G., et al . 2004, ApJ, 613, 898 CrossRefGoogle Scholar