GASP - XVII. H I imaging of the jellyfish galaxy JO206: Gas stripping and enhanced star formation

M. Ramatsoku*, P. Serra, B. M. Poggianti, A. Moretti, M. Gullieuszik, D. Bettoni, T. Deb, J. Fritz, J. H. van Gorkom, Y. L. Jaffé, S. Tonnesen, M. A. W. Verheijen, B. Vulcani, B. Hugo, G. I. G. Józsa, F. M. Maccagni, S. Makhathini, A. Ramaila, O. Smirnov, K. Thorat

*Corresponding author for this work

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Abstract

We present VLA H I observations of JO206, a prototypical ram-pressure- stripped galaxy in the GASP sample. This massive galaxy (M* = 8.5 × 1010 M) is located at a redshift of z = 0.0513, near the centre of the low-mass galaxy cluster, IIZw108 (σ ̃ 575 km s-1). JO206 is characterized by a long tail (≥90 kpc) of ionized gas stripped away by ram pressure. We find a similarly long H I tail in the same direction as the ionized gas tail and measure a total H I mass of 3.2 × 109 M. This is about half the expected H I mass given the stellar mass and surface density of JO206. A total of 1.8 × 109 M (60 per cent) of the detected H I is in the gas-stripped tail. An analysis of the star formation rate shows that the galaxy is forming more stars compared to galaxies with the same stellar and H I mass. On average we find an H I gas depletion time of ̃0.5 Gyr which is about four times shorter than that of `normal' spiral galaxies. We performed a spatially resolved analysis of the relation between star formation rate density and gas density in the disc and tail of the galaxy at the resolution of our H I data. The star formation efficiency of the disc is about 10 times higher than that of the tail at fixed H I surface densities. Both the inner and outer parts of JO206 show an enhanced star formation compared to regions of similar H I surface density in field galaxies. The enhanced star formation is due to ram-pressure stripping during the galaxy's first infall into the cluster.
Original languageEnglish
Pages (from-to)4580-4591
Number of pages12
JournalMonthly Notices of the Royal Astronomical Society
Volume487
Issue number4
DOIs
Publication statusPublished - Aug-2019

Keywords

  • galaxies: clusters: intracluster medium
  • Astrophysics - Astrophysics of Galaxies
  • MORPHOLOGY-DENSITY RELATION
  • ARECIBO SDSS SURVEY
  • RAM-PRESSURE
  • IRREGULAR GALAXIES
  • SPIRAL GALAXIES
  • DISC GALAXIES
  • VIRGO CLUSTER
  • ATOMIC GAS
  • FORMATION EFFICIENCY
  • PHYSICAL-PROPERTIES

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