The ALMaQUEST Survey. VII. Star Formation Scaling Relations of Green Valley Galaxies

Abstract We utilize the ALMA-MaNGA QUEnch and STar formation (ALMaQUEST) survey to investigate the kpc-scale scaling relations, presented as the resolved star-forming MS (rSFMS: Σ SFR versus Σ * ), the resolved Schmidt–Kennicutt relation (rSK: Σ SFR versus Σ H 2 ), and the resolved molecular gas MS...

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Published in:	The Astrophysical journal 2022-02, Vol.926 (2), p.175
Main Authors:	Lin, Lihwai, Ellison, Sara L., Pan, Hsi-An, Thorp, Mallory D., Yu, Po-Chieh, Belfiore, Francesco, Hsieh, Bau-Ching, Maiolino, Roberto, Ramya, S., Sánchez, Sebastián F., Su, Yung-Chau
Format:	Article
Language:	eng
Subjects:	Astronomy & Astrophysics ASTRONOMY AND ASTROPHYSICS Astrophysics Depletion Galaxies Molecular gases Polls & surveys Scaling Star & galaxy formation Star formation Stars & galaxies
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Summary:	Abstract We utilize the ALMA-MaNGA QUEnch and STar formation (ALMaQUEST) survey to investigate the kpc-scale scaling relations, presented as the resolved star-forming MS (rSFMS: Σ SFR versus Σ * ), the resolved Schmidt–Kennicutt relation (rSK: Σ SFR versus Σ H 2 ), and the resolved molecular gas MS (rMGMS: Σ H 2 versus Σ * ), for 11,478 star-forming and 1414 retired spaxels (oversampled by a factor of ∼20) located in 22 GV and 12 MS galaxies. For a given galaxy type (MS or GV), the retired spaxels are found to be offset from the sequences formed by the star-forming spaxels on the rSFMS, rSK, and rMGMS planes, toward lower absolute values of sSFR, SFE, and f H 2 by ∼1.1, 0.6, and 0.5 dex. The scaling relations for GV galaxies are found to be distinct from that of the MS galaxies, even if the analyses are restricted to the star-forming spaxels only. It is found that, for star-forming spaxels, sSFR, SFE, and f H 2 in GV galaxies are reduced by ∼0.36, 0.14, and 0.21 dex, respectively, compared to those in MS galaxies. Therefore, the suppressed sSFR/SFE/ f gas in GV galaxies is associated with not only an increased proportion of retired regions in GV galaxies but also a depletion of these quantities in star-forming regions. Finally, the reduction of SFE and f H 2 in GV galaxies relative to MS galaxies is seen in both bulge and disk regions (albeit with larger uncertainties), suggesting that, statistically, quenching in the GV population may persist from the inner to the outer regions.
ISSN:	0004-637X 1538-4357