The ALMA Detection of Extraplanar 13CO in a Ram-pressure-stripped Galaxy and Its Implication

Bumhyun Lee, Aeree Chung

Research output: Contribution to journalArticle

2 Citations (Scopus)

Abstract

NGC 4522 is a Virgo spiral that is currently undergoing active ram pressure stripping. In previous single-dish observations, 12CO emission was detected outside of the stellar disk, some of which coincides with the extraplanar H i gas and H patches. The extraplanar gas identified in multi-wavelength data makes this galaxy an ideal case to study the impact of pressure due to the cluster medium on the interstellar gas of various phases. In this Letter, we present the high-resolution 12CO(1-0) and 13CO(1-0) data of NGC 4522 obtained using the Atacama Large Millimeter/submillimeter Array (ALMA). In particular, we report here the extraplanar 13CO detection that has never before been seen in ram-pressure-stripped galaxies. As the main donor of 13C in the interstellar medium is evolved stars, the presence of 13CO strongly suggests that heavy elements likely originated from the galactic disk, not from the newly formed stars in situ. Even though it is still inconclusive whether it is stripped in atomic form or as molecules, this study provides evidence for the ram pressure stripping of heavy elements, which can chemically enrich the halo gas, and potentially the intracluster medium, in the case that they are pushed strongly enough to escape the galaxy.

Original languageEnglish
Article numberL10
JournalAstrophysical Journal Letters
Volume866
Issue number1
DOIs
Publication statusPublished - 2018 Oct 10

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ram
galaxies
heavy elements
stripping
gas
gases
stars
interstellar gas
parabolic reflectors
escape
halos
wavelength
detection
high resolution
wavelengths
molecules

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

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abstract = "NGC 4522 is a Virgo spiral that is currently undergoing active ram pressure stripping. In previous single-dish observations, 12CO emission was detected outside of the stellar disk, some of which coincides with the extraplanar H i gas and H patches. The extraplanar gas identified in multi-wavelength data makes this galaxy an ideal case to study the impact of pressure due to the cluster medium on the interstellar gas of various phases. In this Letter, we present the high-resolution 12CO(1-0) and 13CO(1-0) data of NGC 4522 obtained using the Atacama Large Millimeter/submillimeter Array (ALMA). In particular, we report here the extraplanar 13CO detection that has never before been seen in ram-pressure-stripped galaxies. As the main donor of 13C in the interstellar medium is evolved stars, the presence of 13CO strongly suggests that heavy elements likely originated from the galactic disk, not from the newly formed stars in situ. Even though it is still inconclusive whether it is stripped in atomic form or as molecules, this study provides evidence for the ram pressure stripping of heavy elements, which can chemically enrich the halo gas, and potentially the intracluster medium, in the case that they are pushed strongly enough to escape the galaxy.",
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The ALMA Detection of Extraplanar 13CO in a Ram-pressure-stripped Galaxy and Its Implication. / Lee, Bumhyun; Chung, Aeree.

In: Astrophysical Journal Letters, Vol. 866, No. 1, L10, 10.10.2018.

Research output: Contribution to journalArticle

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