@article{9225e952aa554214bdb799b4c1b815ca,
title = "H I content of selected mid-infrared bright, starburst blue compact dwarf galaxies",
abstract = "We report measurements of H I content in 11 nearby, actively star-forming, blue compact dwarf galaxies (BCDs) from 21 cm observations with the Arecibo telescope. These BCDs, selected by their red (W2[4.6 μm]−W3[12 μm]>3.8 mag) and bright mid-infrared (MIR) emission (W4[22 μm]<7.6 mag), have high specific star formation rates (median sSFR ∼10−7.8 yr−1), similar to high redshift galaxies. H I emission was detected in six sources. We analyse our new detections in the context of previous H I observations of 218 dwarf irregulars (dIs) and BCDs in the literature. The MH I–M∗ relation resulting from our observations confirms the dominating fraction of H I gas among baryons in galaxies with lower stellar masses. This Arecibo BCD sample has significantly lower median H I depletion time-scales (τH I ∼ 0.3 Gyr) than other dIs/BCDs (∼ 6.3 Gyr) in the literature. The majority of the sources (10/11) in the Arecibo sample are very red in W1[3.4 μm]−W2[4.6 μm] colour (>0.8 mag) implying the presence of warm dust. We investigate the relation of τHI with stellar mass (M∗) and sSFR. We find that τH I is significantly anticorrelated with M∗ for higher sSFR (>10−8.5 yr−1) and with sSFR for higher stellar mass (> 107.5 M☉) dwarf galaxies. The high sSFR for the BCDs in the Arecibo observed sample is mainly due to their high atomic gas star formation efficiency (SFE) or low τH I. The low τH I or high SFE in these sources is possibly due to runaway star formation in compact and dense super star clusters.",
keywords = "galaxies: dwarf, galaxies: star formation, galaxies: starburst, radio lines: galaxies",
author = "Yogesh Chandola and Di Li and Tsai, \{Chao Wei\} and Guodong Li and Yingjie Peng and Pei Zuo and Travis McIntyre and Ma, \{Yin Zhe\} and Daniel Stern and Roger Griffith and Thomas Jarrett and Peter Eisenhardt and Chantal Balkowski",
note = "Funding Information: This work also makes use of data products from the Panoramic Survey Telescope and Rapid Response System (Pan-STARRS). The Pan-STARRS1 Surveys were made possible through contributions by the Institute for Astronomy, the University of Hawaii, the Pan-STARRS Project Office, the Max-Planck Society and its participating institutes, the Max Planck Institute for Astronomy, Heidelberg and the Max Planck Institute for Extraterrestrial Physics, Garching, The Johns Hopkins University, Durham University, the University of Edinburgh, the Queen{\textquoteright}s University Belfast, the Harvard-Smithsonian Center for Astrophysics, the Las Cumbres Observatory Global Telescope Network Incorporated, the National Central University of Taiwan, the Space Telescope Science Institute, and the National Aeronautics and Space Administration under Grant No. NNX08AR22G issued through the Planetary Science Division of the NASA Science Mission Directorate, the National Science Foundation Grant No. AST-1238877, the University of Maryland, Eotvos Lorand University (ELTE), and the Los Alamos National Laboratory. The Pan-STARRS1 Surveys are archived at the Space Telescope Science Institute (STScI) and can be accessed through MAST, the Mikulski Archive for Space Telescopes. Additional support for the Pan-STARRS1 public science archive is provided by the Gordon and Betty Moore Foundation. This publication makes use of data products from the Wide-Field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory, California Institute of Technology, funded by the National Aeronautics and Space Administration. We thank an anonymous reviewer for useful comments which helped us to improve the paper significantly. This work is supported by the National Natural Science Foundation of China (NSFC) Grant No. 11988101, No. 12050410259, No. 11550110181, No. 11725313, No. 12041302, the International Partnership Program of Chinese Academy of Sciences grant No. 114A11KYSB20160008. YC was sponsored by the Chinese Academy of Sciences Visiting Fellowship for Researchers from Developing Countries, Grant No. 2013FFJB0009, by the FAST distinguished young researcher fellowship (19-FAST-02) from the Center for Astronomical Mega-Science, CAS, and Ministry of Science and Technology (MOST) grant no. QNJ2021061003L. YP acknowledge National Science Foundation of China (NSFC) Grant No. 12125301, 12192220, and 12192222, and the science research grants from the China Manned Space Project with NO. CMS-CSST-2021-A07. YZM acknowledges the support of the National Research Foundation with Grant No. 150580, No. 120385, and No. 120378. Portions of this research were carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. This work also makes use of Sloan Digital Sky Survey (SDSS)-III. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation and the US Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/ . SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington and Yale University. Publisher Copyright: {\textcopyright} The Author(s) 2023. Published by Oxford University Press on behalf of Royal Astronomical Society.",
year = "2024",
month = jan,
day = "1",
doi = "10.1093/mnras/stad3018",
language = "English",
volume = "527",
pages = "603--619",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "Oxford University Press",
number = "1",
}