Compact star forming galaxies as the progenitors of compact quiescent galaxies: clustering result
arXiv:1609.01014 · doi:10.1016/j.newast.2016.08.013
Abstract
We present a measurement of the spatial clustering of massive compact galaxies at in CANDELS/3D-HST fields. We obtain the correlation length for compact quiescent galaxies (cQGs) at of and compact star forming galaxies (cSFGs) at of assuming a power-law slope . The characteristic dark matter halo masses of cQGs at and cSFGs at are and , respectively. Our clustering result suggests that cQGs at are possibly the progenitors of local luminous ETGs and the descendants of cSFGs and SMGs at . Thus an evolutionary connection involving SMGs, cSFGs, QSOs, cQGs and local luminous ETGs has been indicated by our clustering result.
arXiv comment20 pages, 5 figures
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