SDSS-IV MaNGA: The Nature of an Off-galaxy H$α$ Blob -- A Multi-wavelength View of Offset Cooling in a Merging Galaxy Group

Hsi-An Pan, Lihwai Lin, Bau-Ching Hsieh, Michal J. Michalowski, Matthew S. Bothwell, Song Huang, Alexei V. Moiseev, Dmitry Oparin, Ewan O'Sullivan, Diana M. Worrall, Sebastian F. Sanchez, Stephen Gwyn, David R. Law, David V. Stark, Dmitry Bizyaev, Cheng Li, Chien-Hsiu Lee, Hai Fu, Francesco Belfiore, Kevin BundyJose G. Fernandez-Trincado, Joseph Gelfand, Sebastien Peirani

Research output: Contribution to journalArticle (Academic Journal)

Abstract

Galaxies in dense environments, such as groups and clusters, experience various processes by which galaxies gain and lose gas. Using data from the SDSS-IV MaNGA survey, we previously reported the discovery of a giant (6 -- 8 kpc in diameter) H$\alpha$ blob, Totoro, about 8 kpc away from a pair of galaxies (Satsuki and Mei) residing in a galaxy group which is experiencing a group-group merger. Here, we combine interferometric $^{12}$CO(1--0) molecular gas data, new wide-field H$\alpha$, $u$-band data, and published X-ray data to determine the origin of the blob. Several scenarios are discussed to account for its multi-wavelength properties, including (1) H$\alpha$ gas being stripped from galaxy Satsuki by ram-pressure; (2) a separated low-surface-brightness galaxy; (3) gas being ejected or ionized by an active galactic nucleus (AGN); and (4) a cooling intra-group medium (IGM). Scenarios (1) and (2) are less favored by the present data. Scenario (3) is also less likely as there is no evidence for an active ongoing AGN in the host galaxy. We find that the CO (cold) and H$\alpha$ (warm) gas coexist with X-ray (hot) structures; moreover, the derived cooling time is within the regime where molecular and H$\alpha$ gas are expected. The coexistence of gas with different temperatures also agrees with that of cooling gas in other systems. Our multi-wavelength results strongly suggest that the CO and H$\alpha$ gas are the product of cooling from the IGM at its current location, i.e., cooling has occurred, and may be ongoing, well outside the host-galaxy core.
Original languageEnglish
JournalAstrophysical Journal
Publication statusAccepted/In press - 12 Sep 2020

Keywords

  • astro-ph.GA

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