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The growth of the central region by acquisition of counterrotating gas in star-forming galaxies

  • Yan Mei Chen
  • , Yong Shi
  • , Christy A. Tremonti
  • , Matt Bershady
  • , Michael Merrifield
  • , Eric Emsellem
  • , Yi Fei Jin
  • , Song Huang
  • , Hai Fu
  • , David A. Wake
  • , Kevin Bundy
  • , David Stark
  • , Lihwai Lin
  • , Maria Argudo-Fernandez
  • , Thaisa Storchi Bergmann
  • , Dmitry Bizyaev
  • , Joel Brownstein
  • , Martin Bureau
  • , John Chisholm
  • , Niv Drory
  • Qi Guo, Lei Hao, Jian Hu, Cheng Li, Ran Li, Alexandre Roman Lopes, Kai Ke Pan, Rogemar A. Riffel, Daniel Thomas, Lan Wang, Kyle Westfall, Ren Bin Yan

Producción científica: Article › revisión exhaustiva

54 Citas (Scopus)

Resumen

Galaxies grow through both internal and external processes. In about 10% of nearby red galaxies with little star formation, gas and stars are counter-rotating, demonstrating the importance of external gas acquisition in these galaxies. However, systematic studies of such phenomena in blue, star-forming galaxies are rare, leaving uncertain the role of external gas acquisition in driving evolution of blue galaxies. Here, based on new measurements with integral field spectroscopy of a large representative galaxy sample, we find an appreciable fraction of counter-rotators among blue galaxies (9 out of 489 galaxies). The central regions of blue counter-rotators show younger stellar populations and more intense, ongoing star formation than their outer parts, indicating ongoing growth of the central regions. The result offers observational evidence that the acquisition of external gas in blue galaxies is possible; the interaction with pre-existing gas funnels the gas into nuclear regions (<1 kpc) to form new stars.

Idioma originalEnglish
Número de artículo13269
PublicaciónNature Communications
Volumen7
DOI
EstadoPublished - oct 19 2016

Nota bibliográfica

Publisher Copyright:
© The Author(s) 2016.

Financiación

Y.M.C. acknowledges support from NSFC grant 11573013, 11133001, the Natural Science Foundation of Jiangsu Province grant BK20131263, the Opening Project of Key Laboratory of Computational Astrophysics, National Astronomical Observatories, Chinese Academy of Sciences. Y.S. acknowledges support from NSFC grant 11373021, the CAS Pilot-b grant no. XDB09000000 and Jiangsu Scientific Committee grant BK20150014. C.A.T. acknowledges support from National Science Foundation of the United States grant no. 1412287. Funding for the Sloan Digital Sky Survey IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science and the Participating Institutions. SDSS-IV acknowledges support and resources from the Center for High-Performance Computing at the University of Utah.

FinanciadoresNúmero del financiador
University of Utah
U.S. Department of Energy
Opening Project of Key Laboratory of Computational Astrophysics
Alfred P Sloan Foundation
Natural Science Foundation of Jiangsu ProvinceBK20131263
National Science Foundation Arctic Social Science Program1412287
Science and Technology Facilities CouncilST/K00090X/1, ST/N000668/1
Chinese Academy of Sciences11373021, XDB09000000
Jiangsu Scientific CommitteeBK20150014
UK Industrial Decarbonization Research and Innovation Centre53706
National Natural Science Foundation of China (NSFC)11133001

    ASJC Scopus subject areas

    • General Chemistry
    • General Biochemistry, Genetics and Molecular Biology
    • General
    • General Physics and Astronomy

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