Compact and quiescent circumgalactic medium and Ly α haloes around extremely red quasars

Author:

Gillette Jarred1ORCID,Lau Marie Wingyee1ORCID,Hamann Fred1,Perrotta Serena2ORCID,Rupke David S N3ORCID,Wylezalek Dominika4ORCID,Zakamska Nadia L5ORCID,Vayner Andrey5ORCID

Affiliation:

1. Department of Physics & Astronomy, University of California , Riverside, CA 92521 , USA

2. Center for Astrophysics and Space Sciences, University of California , San Diego, CA 92093 , USA

3. Department of Physics, Rhodes College , Memphis, TN 38112 , USA

4. Astronomical Calculation Institute, University of Heidelberg , D-69120 Heidelberg , Germany

5. Department of Physics & Astronomy, Johns Hopkins University , Baltimore, MD 21218 , USA

Abstract

ABSTRACT Red quasars may represent a young stage of galaxy evolution that provide important feedback to their host galaxies. We are studying a population of extremely red quasars (ERQs) with exceptionally fast and powerful outflows, at median redshift z = 2.6. We present Keck/Keck Cosmic Web Imager integral field spectra of 11 ERQs, which have median colour i–W3 = 5.9 mag, median 〈 Lbol 〉 ≈ 5 × 1047 erg s−1, Ly α halo luminosity 〈 Lhalo 〉 = 5 × 1043 erg s−1, and maximum linear size >128 kpc. The ERQ haloes are generally similar to blue quasar haloes, following known trends with Lbol in halo properties. ERQs have halo symmetries similar to Type-I blue quasars, suggesting Type-I spatial orientations. ERQ 〈 Lhalo 〉 is ∼2-dex below blue quasars, which is marginal due to scatter, but consistent with obscuration lowering photon escape fractions. ERQ haloes tend to have more compact and circularly symmetric inner regions than blue quasars, with median exponential scale lengths ∼9 kpc, compared with ∼16 kpc for blue quasars. When we include the central regions not available in blue quasar studies (due to point spread function problems), the true median ERQ halo scale length is just ∼6 kpc. ERQ haloes are kinematically quiet, with median velocity dispersion 293 km s−1, consistent with expected virial speeds. Overall, we find no evidence for feedback on circumgalactic scales, and the current episode of quasar activity (perhaps due to long outflow travel times) has not been around long enough to affect the circumgalactic medium. We confirm the narrow Ly α-emission spikes found in ERQ aperture spectra are halo features, and are useful for systemic redshifts and measuring outflow speeds in other features.

Funder

National Science Foundation

NASA

W. M. Keck Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 1 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. [O iii] λ5007 emissions in extremely red quasars (ERQs) are compact;Monthly Notices of the Royal Astronomical Society;2024-07-01

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