MaNGA 8313-1901: gas accretion observed in a blue compact dwarf galaxy?
Mengting Ju, Jun Yin, Rongrong Liu, Lei Hao, Zhengyi Shao, Shuai Feng,, Rog\'erio Riffel, Chenxu Liu, David V. Stark, Shiyin Shen, Eduardo Telles,, Jos\'e G. Fern\'andez-Trincado, Junfeng Wang, Haiguang Xu, Dmitry Bizyaev, Yu, Rong

TL;DR
This study presents observational evidence of gas accretion in a Blue Compact Dwarf galaxy, highlighting a low-metallicity, star-forming clump with detached gas kinematics, suggesting external gas inflow rather than internal processes.
Contribution
First direct observational evidence of ongoing gas accretion in a BCD galaxy, identified through distinct kinematic and metallicity features of an off-centered clump.
Findings
Detection of a low-metallicity, star-forming NE clump with detached gas kinematics.
Spectral analysis indicates recent star formation from accreted cold gas.
Potential shared origin of gas accretion for multiple clumps.
Abstract
Gas accretion is an important process in the evolution of galaxies, but it has limited direct observational evidences. In this paper, we report the detection of a possible ongoing gas accretion event in a Blue Compact Dwarf (BCD) galaxy, MaNGA 8313-1901, observed by the Mapping Nearby Galaxies and Apache Point Observatory (MaNGA) program. This galaxy has a distinct off-centered blue clump to the northeast (the NE clump) that shows low metallicity and enhanced star-formation. The kinematics of the gas in the NE clump also seems to be detached from the host BCD galaxy. Together with the metallicity drop of the NE clump, it suggests that the NE clump likely has an external origin, such as the gas accretion or galaxy interaction, rather than an internal origin, such as an \hii~complex in the disk. After removing the underlying host component, we find that the spectrum of the "pure" clump…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astrophysics and Star Formation Studies · Stellar, planetary, and galactic studies
