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Lyman continuum leakage from low-mass galaxies with M ⋆ < 108 M⊙

Journal Article · · Monthly Notices of the Royal Astronomical Society
 [1];  [2];  [3];  [1];  [4];  [5];  [6];  [7]
  1. Bogolyubov Institute for Theoretical Physics, National Academy of Sciences of Ukraine, 14-b Metrolohichna str., Kyiv UA-03143, Ukraine
  2. Institut für Physik und Astronomie, Universität Potsdam, Karl-Liebknecht-Str. 24/25, D-14476 Potsdam, Germany
  3. Observatoire de Genève, Université de Genève, 51 Ch. des Maillettes, CH-1290 Versoix, Switzerland, IRAP/CNRS, 14, Av. E. Belin, F-31400 Toulouse, France
  4. Astronomy Department, University of Texas at Austin, 2515 Speedway, Stop C1400 Austin, TX 78712-1205, USA
  5. Astronomy Department, University of Virginia, P.O. Box 400325, Charlottesville, VA 22904-4325, USA
  6. Institut für Astrophysik, Göttingen Universität, Friedrich-Hund-Platz 1, D-37077 Göttingen, Germany
  7. Observatoire de Genève, Université de Genève, 51 Ch. des Maillettes, CH-1290 Versoix, Switzerland
ABSTRACT

We present observations with the Cosmic Origins Spectrograph onboard the Hubble Space Telescope of nine low-mass star-forming galaxies at redshifts, z, in the range 0.3179–0.4524, with stellar masses $$M_\star \, \lt $$ 108 M⊙ and very high specific star-formation rates sSFR ∼150–630 Gyr−1, aiming to study the dependence of leaking Lyman continuum (LyC) emission on stellar mass and some other characteristics of the galaxy. We detect LyC emission in four out of nine galaxies with escape fractions, fesc(LyC), in the range of 11–35 per cent, and establish upper limits for fesc(LyC) in the remaining five galaxies. We observe a narrow Ly α emission line with two peaks in seven galaxies and likely more complex Ly α profiles in the two remaining galaxies. The velocity separation between the peaks Vsep varies in the range from ∼229 to ∼512 km s−1. Our additional data on low-mass galaxies confirm and strengthen the tight anticorrelation between fesc(LyC) and Vsep found for previous low-redshift galaxy samples with higher stellar masses. Vsep remains the best indirect indicator of LyC leakage. It is better than O32 on which fesc(LyC) depends weakly, with a large scatter. Finally, contrary to expectations, we find no increase of fesc(LyC) with decreasing galaxy stellar mass M⋆.

Sponsoring Organization:
USDOE
OSTI ID:
1772150
Journal Information:
Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 2 Vol. 503; ISSN 0035-8711
Publisher:
Oxford University PressCopyright Statement
Country of Publication:
United Kingdom
Language:
English

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