Search Publications

Radio Jet Proper-motion Analysis of Nine Distant Quasars above Redshift 3.5
DOI: 10.3847/1538-4357/ac87f8 Bibcode: 2022ApJ...937...19Z

Frey, Sándor; Gabányi, Krisztina Éva; An, Tao +2 more

Up to now, jet kinematic studies of radio quasars have barely reached beyond the redshift range z > 3.5. This significantly limits our knowledge of high-redshift jets, which can provide key information for understanding the jet nature and the growth of black holes in the early universe. In this paper, we selected nine radio-loud quasars at z &g…

2022 The Astrophysical Journal
Gaia 10
A Quarter Century of Guitar Nebula/Filament Evolution
DOI: 10.3847/1538-4357/ac9794 Bibcode: 2022ApJ...939...70D

Kargaltsev, Oleg; Klingler, Noel; Slane, Patrick +6 more

We have collected a new deep Chandra X-Ray Observatory exposure of PSR B2224+65 and the "Guitar Nebula," mapping the complex X-ray structure. This is accompanied by a new Hubble Space Telescope (HST) Hα image of the head of the Guitar. Comparing the HST and Chandra structures in four epochs over 25 yr, we constrain the evolution of the TeV particl…

2022 The Astrophysical Journal
Gaia eHST 10
The Dark Matter Halo of M54
DOI: 10.3847/1538-4357/ac7d54 Bibcode: 2022ApJ...935...14C

Grillmair, Carl J.; Carlberg, Raymond G.

M54 is a prototype for a globular cluster embedded in a dark matter halo. Gaia Early Data Release 3 photometry and proper motions separate the old, metal-poor stars from the more metal-rich and younger dwarf galaxy stars. The metal-poor stars dominate the inner 50 pc, with a velocity dispersion profile that declines to a minimum around 30 pc then …

2022 The Astrophysical Journal
Gaia 10
LARS XIII: High Angular Resolution 21 cm H I Observations of Lyα Emitting Galaxies
DOI: 10.3847/1538-4357/ac77ed Bibcode: 2022ApJ...934...69L

Cannon, John M.; Hayes, Matthew; Östlin, Göran +8 more

The Lyα emission line is one of the main observables of galaxies at high redshift, but its output depends strongly on the neutral gas distribution and kinematics around the star-forming regions where UV photons are produced. We present observations of Lyα and 21 cm H I emission at comparable scales with the goal to qualitatively investigate how th…

2022 The Astrophysical Journal
eHST 10
Optical-Radio Position Offsets Are Inversely Correlated with AGN Photometric Variability
DOI: 10.3847/2041-8213/ac8d5d Bibcode: 2022ApJ...939L..32S

Secrest, Nathan J.

Using photometric variability information from the new Gaia DR3 release, I show for the first time that photometric variability is inversely correlated with the prevalence of optical-radio position offsets in the active galactic nuclei (AGNs) that comprise the International Celestial Reference Frame (ICRF). While the overall prevalence of statisti…

2022 The Astrophysical Journal
Gaia 10
Connecting Low- and High-redshift Weak Emission-line Quasars via Hubble Space Telescope Spectroscopy of Lyα Emission
DOI: 10.3847/1538-4357/ac5bd6 Bibcode: 2022ApJ...929...78P

Brandt, W. N.; Anderson, Scott F.; Fan, Xiaohui +10 more

We present ultraviolet spectroscopy covering the Lyα + N V complex of six candidate low-redshift (0.9 < z < 1.5) weak emission-line quasars (WLQs) based on observations with the Hubble Space Telescope. The original systematic searches for these puzzling Type 1 quasars with intrinsically weak broad emission lines revealed an N ≈ 100 WLQ popul…

2022 The Astrophysical Journal
eHST 9
SKYSURF-3: Testing Crowded Object Catalogs in the Hubble eXtreme Deep Field Mosaics to Study Sample Incompleteness from an Extragalactic Background Light Perspective
DOI: 10.3847/2041-8213/ac9cca Bibcode: 2022ApJ...940L..15K

Pirzkal, Nor; Windhorst, Rogier A.; Koekemoer, Anton +6 more

Extragalactic background light (EBL) studies have revealed a significant discrepancy between direct measurements-via instruments measuring "bare" sky from which Zodiacal and Galactic light models are subtracted-and measurements of the integrated galaxy light (IGL). This discrepancy could lie in either method, whether it be an incomplete Zodiacal m…

2022 The Astrophysical Journal
eHST 9
A Star-sized Impact-produced Dust Clump in the Terrestrial Zone of the HD 166191 System
DOI: 10.3847/1538-4357/ac4bbb Bibcode: 2022ApJ...927..135S

Rieke, G. H.; Kennedy, Grant M.; Su, Kate Y. L. +2 more

We report on five years of 3-5 µm photometry measurements obtained by warm Spitzer to track the dust debris emission in the terrestrial zone of HD 166191 in combination with simultaneous optical data. We show that the debris production in this young (~10 Myr) system increased significantly in early 2018 and reached a record high level (almos…

2022 The Astrophysical Journal
Gaia 9
Radio Observations of Four Active Galactic Nuclei Hosting Intermediate-mass Black Hole Candidates: Studying the Outflow Activity and Evolution
DOI: 10.3847/1538-4357/ac9e9d Bibcode: 2022ApJ...941...43Y

Ho, Luis C.; Zhang, Shaohua; Yang, Jun +5 more

Observational searches for intermediate-mass black holes (IMBHs; 102-106 M ) include relatively isolated dwarf galaxies. For those that host active galactic nuclei (AGNs), the IMBH nature may be discerned through the accretion-jet activity. We present radio observations of four AGN-hosting dwarf galaxies, which po…

2022 The Astrophysical Journal
Gaia 9
Far-ultraviolet Flares on Accreting Protostars: Weak and Classical T Tauri Stellar Pair Analysis
DOI: 10.3847/1538-4357/ac8f26 Bibcode: 2022ApJ...939...82H

Kowalski, Adam F.; France, Kevin; Hinton, P. C. +5 more

The far-ultraviolet (FUV) emission of classical T Tauri stars (CTTSs) is known to play an important role in protoplanetary disk dispersal and giant planet formation, yet the role played by protostellar flares in these processes is largely unknown. We use nearby star-forming regions as laboratories to probe the FUV flare characteristics of CTTSs an…

2022 The Astrophysical Journal
eHST 9