Distribution of Faint Atomic Gas in Hickson Compact Groups
Sanchayeeta Borthakur, Min S. Yun, Lourdes Verdes-Montenegro, Timothy, M. Heckman, Guangtun Zhu, James A. Braatz

TL;DR
This study uses 21cm HI observations to map faint atomic gas in Hickson Compact Groups, revealing its distribution, origin, and survival timescales, thus enhancing understanding of intragroup medium properties.
Contribution
It provides new estimates of HI masses in HCGs using GBT, detecting more diffuse gas than previous VLA imaging and analyzing its spatial distribution and origin.
Findings
Detected 65% more HI with GBT than VLA in HCG92.
Faint gas in some groups shares spatial distribution with high-surface brightness HI.
Faint gas is likely of tidal origin and can remain neutral for at least 500 Myrs.
Abstract
We present 21cm HI observations of four Hickson Compact Groups with evidence for a substantial intragroup medium using the Robert C. Byrd Green Bank Telescope (GBT). By mapping H I emission in a region of 2525 (140-650 kpc) surrounding each HCG, these observations provide better estimates of HI masses. In particular, we detected 65% more \HI than that detected in the Karl G. Jansky Very Large Array (VLA) imaging of HCG92. We also identify if the diffuse gas has the same spatial distribution as the high-surface brightness (HSB) HI features detected in the VLA maps of these groups by comparing the HI strengths between the observed and modeled masses based on VLA maps. We found that the HI observed with the GBT to have a similar spatial distribution as the HSB structures in HCGs 31 and 68. Conversely, the observed HI distributions in HCGs44 and 92 were extended…
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