What if young<i>z</i>&amp;gt; 9<i>JWST</i>galaxies hosted massive black holes?

نویسندگان

چکیده

JWST is discovering star forming `candidate' galaxies with photometric redshifts $z>9$ and little attenuation. We model presumptive massive black holes (MBHs) in such find that their unobscured emission fainter than the galaxy starlight filters, difficult to be detected via color-color selection, X-ray radio observations. Only MBHs overmassive relative expected scaling relations, accreting at high Eddington rates, would detectable. Their discovery point presence of heavy MBH seeds, but care needed exclude existence lighter seeds as only are detectable this type galaxies. Conversely, if no hosted these galaxies, either there or they rare. The most massive/highest redshift candidate can attain stellar masses excess 5e10 Msun by z~6 grow along SFR-mass sequence, nurse a growing from ~1e5 up >3e7 z~6, become hosts some z>6 quasars. Candidate log(M_{gal}/Msun)~8 not putative fast, unless >1e6 Msun. number density far outnumbers highest-z quasar allows for about 1 bright z~6-7 every 1000

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ژورنال

عنوان ژورنال: Monthly Notices of the Royal Astronomical Society

سال: 2023

ISSN: ['0035-8711', '1365-8711', '1365-2966']

DOI: https://doi.org/10.1093/mnras/stad499