1. Sizes and mass profiles of candidate massive galaxies discovered by JWST at 7
- Author
-
Baggen, Josephine F. W., van Dokkum, Pieter, Labbe, Ivo, Brammer, Gabriel, Miller, Tim B., Bezanson, Rachel, Leja, Joel, Wang, Bingjie, Whitaker, Katherine E., Suess, Katherine A., and Nelson, Erica J.
- Subjects
Astrophysics of Galaxies (astro-ph.GA) ,FOS: Physical sciences - Abstract
The first JWST data revealed an unexpected population of red galaxies that appear to have redshifts of $z\sim 7-9$ and high masses of $M_*$ $\sim$ 10$^{10}$ M$_{\odot}$ (Labbé et al. 2023). Here we fit Sérsic profiles to the F200W NIRCam images of the 13 massive galaxy candidates of Labbé et al., to determine their structural parameters. Satisfactory fits were obtained for nine galaxies. We find that their effective radii are extremely small, ranging from $r_{\rm e}\sim 80$ pc to $r_{\rm e} \sim 300$ pc, with a mean of $\langle r_{\rm e}\rangle \approx 150$ pc. For their apparent stellar masses, the galaxies are smaller than any other galaxy population that has been observed at any other redshift. We use the fits to derive circularized three-dimensional stellar mass profiles of the galaxies, and compare these to the mass profiles of massive quiescent galaxies at $z\sim$2.3 and nearby elliptical galaxies. We find that, despite the high redshift galaxies having $10-20$ times smaller half-light radii, the central stellar densities are comparable to those of their putative descendants at later times. The most straightforward interpretation is that the dense compact inner regions of the most massive ellipticals today were already in place $\sim 600$ Myr after the Big Bang. We caution that the redshifts and masses of the galaxies remain to be confirmed, and that the complex NIRCam point spread function is not yet fully characterized., Submitted to ApJ Letters
- Published
- 2023
- Full Text
- View/download PDF