Search Publications

Evolution of the Thermodynamic Properties of Clusters of Galaxies out to Redshift of 1.8
DOI: 10.3847/1538-4357/abc68d Bibcode: 2021ApJ...910...14G

Mahler, Guillaume; Kraft, Ralph; Khullar, Gourav +11 more

The thermodynamic properties of the hot plasma in galaxy clusters retain information on the processes leading to the formation and evolution of the gas in their deep, dark matter potential wells. These processes are dictated not only by gravity but also by gas physics, e.g., active galactic nucleus feedback and turbulence. In this work, we study t…

2021 The Astrophysical Journal
XMM-Newton 33
The Mass-Metallicity Relation at z 1-2 and Its Dependence on the Star Formation Rate
DOI: 10.3847/1538-4357/ac1105 Bibcode: 2021ApJ...919..143H

Papovich, Casey; Barro, Guillermo; Martin, Crystal L. +24 more

We present a new measurement of the gas-phase mass-metallicity relation (MZR) and its dependence on star formation rates (SFRs) at 1.3 < z < 2.3. Our sample comprises 1056 galaxies with a mean redshift of z = 1.9, identified from the Hubble Space Telescope Wide Field Camera 3 (WFC3) grism spectroscopy in the Cosmic Assembly Near-infrared Dee…

2021 The Astrophysical Journal
eHST 33
Measuring and Replicating the 1-20 µm Energy Distributions of the Coldest Brown Dwarfs: Rotating, Turbulent, and Nonadiabatic Atmospheres
DOI: 10.3847/1538-4357/ac0cfe Bibcode: 2021ApJ...918...11L

Marley, Mark; Dupuy, Trent J.; Caselden, Dan +7 more

Cold, low-mass, field brown dwarfs are important for constraining the terminus of the stellar mass function, and also for optimizing atmospheric studies of exoplanets. In 2020 new model grids for such objects were made available: Sonora-Bobcat and ATMO 2020. Also, new candidate cold brown dwarfs were announced, and new spectroscopic observations a…

2021 The Astrophysical Journal
Gaia 33
Threaded-field-line Model for the Low Solar Corona Powered by the Alfvén Wave Turbulence
DOI: 10.3847/1538-4357/abc000 Bibcode: 2021ApJ...908..172S

Jin, Meng; Sokolov, Igor V.; Gombosi, Tamas I. +6 more

We present an updated global model of the solar corona, including the transition region. We simulate the realistic three-dimensional (3D) magnetic field using the data from the photospheric magnetic field measurements and assume the magnetohydrodynamic (MHD) Alfvén wave turbulence and its nonlinear dissipation to be the only source for heating the…

2021 The Astrophysical Journal
Ulysses 33
The JCMT BISTRO Survey: Revealing the Diverse Magnetic Field Morphologies in Taurus Dense Cores with Sensitive Submillimeter Polarimetry
DOI: 10.3847/2041-8213/abeb1c Bibcode: 2021ApJ...912L..27E

Zhang, Yapeng; Pattle, Kate; Ward-Thompson, Derek +142 more

We have obtained sensitive dust continuum polarization observations at 850 µm in the B213 region of Taurus using POL-2 on SCUBA-2 at the James Clerk Maxwell Telescope as part of the B-fields in STar-forming Region Observations (BISTRO) survey. These observations allow us to probe magnetic field (B-field) at high spatial resolution (∼2000 au …

2021 The Astrophysical Journal
Herschel 32
Disruption of Hierarchical Clustering in the Vela OB2 Complex and the Cluster Pair Collinder 135 and UBC 7 with Gaia EDR3: Evidence of Supernova Quenching
DOI: 10.3847/1538-4357/ac2838 Bibcode: 2021ApJ...923...20P

Tang, Shih-Yun; Hong, Jongsuk; Pang, Xiaoying +4 more

We identify hierarchical structures in the Vela OB2 complex and the cluster pair Collinder 135 and UBC 7 with Gaia EDR3 using the neural network machine-learning algorithm StarGO. Five second-level substructures are disentangled in Vela OB2, which are referred to as Huluwa 1 (Gamma Velorum), Huluwa 2, Huluwa 3, Huluwa 4, and Huluwa 5. For the firs…

2021 The Astrophysical Journal
Gaia 32
Flux Ropes, Turbulence, and Collisionless Perpendicular Shock Waves: High Plasma Beta Case
DOI: 10.3847/1538-4357/abf7c8 Bibcode: 2021ApJ...913..127Z

Zhao, L. L.; Zank, G. P.; Adhikari, L. +4 more

With the onset of solar maximum and the expected increased prevalence of interplanetary shock waves, Parker Solar Probe is likely to observe numerous shocks in the next few years. An outstanding question that has received surprisingly little attention has been how turbulence interacts with collisionless shock waves. Turbulence in the supersonic so…

2021 The Astrophysical Journal
Ulysses 32
Searches after Gravitational Waves Using ARizona Observatories (SAGUARO): Observations and Analysis from Advanced LIGO/Virgo's Third Observing Run
DOI: 10.3847/1538-4357/abeb71 Bibcode: 2021ApJ...912..128P

Gabor, P.; Smith, N.; Rest, A. +35 more

With the conclusion of the third observing run for Advanced LIGO/Virgo (O3), we present a detailed analysis of both triggered and serendipitous observations of 17 gravitational-wave (GW) events (7 triggered and 10 purely serendipitous) from the Searches After Gravitational-waves Using ARizona Observatories (SAGUARO) program. We searched a total of…

2021 The Astrophysical Journal
Gaia 32
The Complex Organic Molecular Content in the L1498 Starless Core
DOI: 10.3847/1538-4357/ac024c Bibcode: 2021ApJ...917...44J

Caselli, Paola; Viti, Serena; Jiménez-Serra, Izaskun +3 more

Observations carried out toward starless and prestellar cores have revealed that complex organic molecules are prevalent in these objects, but it is unclear what chemical processes are involved in their formation. Recently, it has been shown that complex organics are preferentially produced at an intermediate-density shell within the L1544 prestel…

2021 The Astrophysical Journal
Herschel 32
Galaxy Mergers up to z < 2.5. II. AGN Incidence in Merging Galaxies at Separations of 3-15 kpc
DOI: 10.3847/1538-4357/abdbb1 Bibcode: 2021ApJ...909..124S

Marchesini, Danilo; Iono, Daisuke; Silverman, John D. +4 more

We present a study of the incidence of active galactic nucleus (AGN) in a sample of major merging systems at 0.3 < z < 2.5. Galaxies in this merger sample have projected separations between 3 and 15 kpc and are selected from the CANDELS/3D-Hubble Space Telescope catalogs using a peak-finding algorithm. AGNs in mergers and non-mergers are ide…

2021 The Astrophysical Journal
eHST 32