Rights statement: This is an author-created, un-copyedited version of an article accepted for publication/published in The Astrophysical Journal. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at doi:10.3847/0004-637X/832/2/182
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Research output: Contribution to Journal/Magazine › Journal article › peer-review
Research output: Contribution to Journal/Magazine › Journal article › peer-review
}
TY - JOUR
T1 - SDSS-IV MaNGA
T2 - a serendipitous observation of a potential gas accretion event
AU - Cheung, Edmond
AU - Stark, David V.
AU - Huang, Song
AU - Rubin, Kate H. R.
AU - Lin, Lihwai
AU - Tremonti, Christy
AU - Zhang, Kai
AU - Yan, Renbin
AU - Bizyaev, Dmitry
AU - Boquien, Mederic
AU - Brownstein, Joel R.
AU - Drory, Niv
AU - Gelfand, Joseph D.
AU - Knapen, Johan H.
AU - Maiolino, Roberto
AU - Malanushenko, Olena
AU - Masters, Karen L.
AU - Merrifield, Michael R.
AU - Pace, Zach
AU - Pan, Kaike
AU - Riffel, Rogemar A.
AU - Roman-Lopes, Alexandre
AU - Rujopakarn, Wiphu
AU - Schneider, Donald P.
AU - Stott, John P.
AU - Thomas, Daniel
AU - Weijmans, Anne-Marie
N1 - This is an author-created, un-copyedited version of an article accepted for publication/published in The Astrophysical Journal. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at doi:10.3847/0004-637X/832/2/182
PY - 2016/12/1
Y1 - 2016/12/1
N2 - The nature of warm, ionized gas outside of galaxies may illuminate several key galaxy evolutionary processes. A serendipitous observation by the MaNGA survey has revealed a large, asymmetric H alpha complex with no optical counterpart that extends approximate to 8 '' (approximate to 6.3 kpc) beyond the effective radius of a dusty, starbursting galaxy. This H alpha extension is approximately three times the effective radius of the host galaxy and displays a tail-like morphology. We analyze its gas- phase metallicities, gaseous kinematics, and emission- line ratios and discuss whether this Ha extension could be diffuse ionized gas, a gas accretion event, or something else. We find that this warm, ionized gas structure is most consistent with gas accretion through recycled wind material, which could be an important process that regulates the low- mass end of the galaxy stellar mass function.
AB - The nature of warm, ionized gas outside of galaxies may illuminate several key galaxy evolutionary processes. A serendipitous observation by the MaNGA survey has revealed a large, asymmetric H alpha complex with no optical counterpart that extends approximate to 8 '' (approximate to 6.3 kpc) beyond the effective radius of a dusty, starbursting galaxy. This H alpha extension is approximately three times the effective radius of the host galaxy and displays a tail-like morphology. We analyze its gas- phase metallicities, gaseous kinematics, and emission- line ratios and discuss whether this Ha extension could be diffuse ionized gas, a gas accretion event, or something else. We find that this warm, ionized gas structure is most consistent with gas accretion through recycled wind material, which could be an important process that regulates the low- mass end of the galaxy stellar mass function.
KW - galaxies: abundances
KW - galaxies: evolution
KW - galaxies: formation
KW - galaxies: starburst
KW - DIFFUSE IONIZED-GAS
KW - DIGITAL SKY SURVEY
KW - STAR-FORMING GALAXIES
KW - ULTRA DEEP FIELD
KW - H-II REGIONS
KW - REDSHIFT CIRCUMGALACTIC MEDIUM
KW - STELLAR POPULATION SYNTHESIS
KW - LOCAL TADPOLE GALAXIES
KW - LAMBDA-CDM UNIVERSE
KW - ON SPIRAL GALAXIES
U2 - 10.3847/0004-637X/832/2/182
DO - 10.3847/0004-637X/832/2/182
M3 - Journal article
VL - 832
JO - The Astrophysical Journal
JF - The Astrophysical Journal
SN - 0004-637X
IS - 2
M1 - 182
ER -