Bibcode
Puglisi, A.; Daddi, E.; Liu, D.; Bournaud, F.; Silverman, J. D.; Circosta, C.; Calabrò, A.; Aravena, M.; Cibinel, A.; Dannerbauer, H.; Delvecchio, I.; Elbaz, D.; Gao, Y.; Gobat, R.; Jin, S.; Le Floc’h, E.; Magdis, G. E.; Mancini, C.; Riechers, D. A.; Rodighiero, G.; Sargent, M.; Valentino, F.; Zanisi, L.
Referencia bibliográfica
The Astrophysical Journal Letters, Volume 877, Issue 2, article id. L23, 6 pp. (2019).
Fecha de publicación:
6
2019
Número de citas
53
Número de citas referidas
52
Descripción
Atacama Large Millimeter/submillimeter Array (ALMA) measurements for 93
Herschel-selected galaxies at 1.1 ≤ z ≤ 1.7 in COSMOS reveal a
sizable (>29%) population with compact star formation (SF) sizes,
lying on average >×3.6 below the optical stellar mass (M
⋆)–size relation of disks. This sample widely
spans the star-forming main sequence (MS), having 108 ≤ M
⋆ ≤ 1011.5 M ⊙ and 20 ≤
star formation rate (SFR) ≤ 680 M ⊙
yr‑1. The 32 size measurements and 61 upper limits are
measured on ALMA images that combine observations of CO(5–4),
CO(4–3), CO(2–1), and λ obs ∼
1.1–1.3 mm continuum, all tracing the star-forming molecular gas.
These compact galaxies have instead normally extended K band
sizes, suggesting strong specific SFR gradients. Compact galaxies
comprise the 50 ± 18% of MS galaxies at M ⋆ >
1011 M ⊙. This is not expected in standard
bimodal scenarios, where MS galaxies are mostly steadily growing
extended disks. We suggest that compact MS objects are early
post-starburst galaxies in which the merger-driven boost of SF has
subsided. They retain their compact SF size until either further gas
accretion restores premerger galaxy-wide SF, or until becoming quenched.
The fraction of merger-affected SF inside the MS seems thus larger than
anticipated and might reach ∼50% at the highest M ⋆.
The presence of large galaxies above the MS demonstrates an overall poor
correlation between galaxy SF size and specific SFR.
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