Search Publications

Intracluster Magnetic Filaments and an Encounter with a Radio Jet
DOI: 10.3847/1538-4357/ac7c76 Bibcode: 2022ApJ...935..168R

Brunetti, G.; Forman, W.; Jones, T. W. +6 more

Thin synchrotron-emitting filaments are increasingly seen in the intracluster medium (ICM). We present the first example of a direct interaction between a magnetic filament, a radio jet, and a dense ICM clump in the poor cluster A194. This enables the first exploration of the dynamics and possible histories of magnetic fields and cosmic rays in su…

2022 The Astrophysical Journal
XMM-Newton 37
BASS XXXII: Studying the Nuclear Millimeter-wave Continuum Emission of AGNs with ALMA at Scales ≲100-200 pc
DOI: 10.3847/1538-4357/ac8794 Bibcode: 2022ApJ...938...87K

Baba, Shunsuke; Imanishi, Masatoshi; Ueda, Yoshihiro +25 more

To understand the origin of nuclear (≲100 pc) millimeter-wave (mm-wave) continuum emission in active galactic nuclei (AGNs), we systematically analyzed subarcsecond resolution Band-6 (211-275 GHz) Atacama Large Millimeter/submillimeter Array data of 98 nearby AGNs (z < 0.05) from the 70 month Swift/BAT catalog. The sample, almost unbiased for o…

2022 The Astrophysical Journal
AKARI Herschel 37
ALMA Observations of NGC 6334S. II. Subsonic and Transonic Narrow Filaments in a High-mass Star Formation Cloud
DOI: 10.3847/1538-4357/ac3df8 Bibcode: 2022ApJ...926..165L

Sanhueza, Patricio; Smith, Howard A.; Qiu, Keping +21 more

We present a study of narrow filaments toward a massive infrared dark cloud, NGC 6334S, using the Atacama Large Millimeter/submillimeter Array. Thirteen gas filaments are identified using the H13CO+ line, while a single continuum filament is revealed by the continuum emission. The filaments present a compact radial distributi…

2022 The Astrophysical Journal
Herschel 37
First Peek with JWST/NIRCam Wide-field Slitless Spectroscopy: Serendipitous Discovery of a Strong [O III]/Hα Emitter at z = 6.11
DOI: 10.3847/2041-8213/ac8938 Bibcode: 2022ApJ...936L...8S

Koekemoer, Anton M.; Pirzkal, Nor; Gennaro, Mario +16 more

We report the serendipitous discovery of an [O III] λ λ4959/5007 and Hα line emitter in the Epoch of Reionization (EoR) with the James Webb Space Telescope (JWST) commissioning data taken in the NIRCam wide-field slitless spectroscopy (WFSS) mode. Located ~55″ away from the flux calibrator P330-E, this galaxy exhibits bright [O III] λ λ4959/5007 a…

2022 The Astrophysical Journal
Gaia JWST 37
Predicting Solar Flares Using CNN and LSTM on Two Solar Cycles of Active Region Data
DOI: 10.3847/1538-4357/ac64a6 Bibcode: 2022ApJ...931..163S

Chen, Yang; Gombosi, Tamas; Bobra, Monica G. +5 more

We consider the flare prediction problem that distinguishes flare-imminent active regions that produce an M- or X-class flare in the succeeding 24 hr, from quiet active regions that do not produce any flares within ±24 hr. Using line-of-sight magnetograms and parameters of active regions in two data products covering Solar Cycles 23 and 24, we tra…

2022 The Astrophysical Journal
SOHO 36
Evolution of a Relativistic Outflow and X-Ray Corona in the Extreme Changing-look AGN 1ES 1927+654
DOI: 10.3847/1538-4357/ac76c0 Bibcode: 2022ApJ...934...35M

Fabian, Andrew C.; Remillard, Ronald A.; Ricci, Claudio +8 more

1ES 1927+654 is a paradigm-defying active galactic nucleus (AGN) and one of the most peculiar X-ray nuclear transients. In early 2018, this well-known AGN underwent a changing-look event, in which broad optical emission lines appeared and the optical flux increased. Yet, by 2018 July, the X-ray flux had dropped by over two orders of magnitude, ind…

2022 The Astrophysical Journal
XMM-Newton 36
CO Line Emission Surfaces and Vertical Structure in Midinclination Protoplanetary Disks
DOI: 10.3847/1538-4357/ac6c02 Bibcode: 2022ApJ...932..114L

Wilner, David J.; Ilee, John D.; Andrews, Sean M. +18 more

High spatial resolution CO observations of midinclination (≈30°-75°) protoplanetary disks offer an opportunity to study the vertical distribution of CO emission and temperature. The asymmetry of line emission relative to the disk major axis allows for a direct mapping of the emission height above the midplane, and for optically thick, spatially re…

2022 The Astrophysical Journal
Gaia 36
Metallicities of Five z > 5 Emission-line Galaxies in SMACS 0723 Revealed by JWST
DOI: 10.3847/2041-8213/ac959d Bibcode: 2022ApJ...939L...3T

Barger, A. J.; Cowie, L. L.; Taylor, A. J.

JWST's Early Release Observations of the lensing cluster SMACS J0723.3-7327 have given an unprecedented spectroscopic look into the high-redshift universe. These observations reveal five galaxies at z > 5. All five have detectable [O III]λ4363 line emission, indicating that these galaxies have high temperatures and low metallicities and that th…

2022 The Astrophysical Journal
JWST 36
JWST Sneaks a Peek at the Stellar Morphology of z 2 Submillimeter Galaxies: Bulge Formation at Cosmic Noon
DOI: 10.3847/2041-8213/ac98c6 Bibcode: 2022ApJ...939L...7C

Smail, Ian; Chen, Chian-Chou; Wang, Wei-Hao +6 more

We report morphological analyses of seven submillimeter galaxies (SMGs) at z ~ 2 using the James Webb Space Telescope NIRCam images taken as part of the public CEERS and PRIMER surveys. Through two-dimensional surface brightness profile fitting we find evidence of compact reddened stellar structures in all the SMGs, in particular in the F444W filt…

2022 The Astrophysical Journal
Gaia eHST JWST 36
Evidence for Cold-stream to Hot-accretion Transition as Traced by Lyα Emission from Groups and Clusters at 2 < z < 3.3
DOI: 10.3847/2041-8213/ac531f Bibcode: 2022ApJ...926L..21D

Finoguenov, A.; Daddi, E.; Elbaz, D. +12 more

We present Keck Cosmic Web Imager observations of giant Lyα halos surrounding nine galaxy groups and clusters at 2 < z < 3.3, including five new detections and one upper limit. We find observational evidence for the cold-stream to hot-accretion transition predicted by theory by measuring a decrease in the ratio between the spatially extended…

2022 The Astrophysical Journal
eHST 35