Search Publications

On the Origin of Radio-loudness in Active Galactic Nuclei Using Far-infrared Polarimetric Observations
DOI: 10.3847/1538-4357/accb96 Bibcode: 2023ApJ...951...31L

Lopez-Rodriguez, Enrique; Blandford, Roger; Begelman, Mitchell C. +3 more

The dichotomy between radio-loud (RL) and radio-quiet (RQ) active galactic nuclei (AGNs) is thought to be intrinsically related to radio jet production. This difference may be explained by the presence of a strong magnetic field (B-field) that enhances, or is the cause of, the accretion activity and the jet power. Here we report the first evidence…

2023 The Astrophysical Journal
Herschel eHST 7
CGM2 + CASBaH: The Mass Dependence of H I Lyα-Galaxy Clustering and the Extent of the CGM
DOI: 10.3847/1538-4357/acc85b Bibcode: 2023ApJ...948..114W

Tripp, Todd M.; Prochaska, J. Xavier; Tejos, Nicolas +9 more

We combine data sets from the CGM2 and CASBaH surveys to model a transition point, R cross, between circumgalactic and intergalactic media (CGM and IGM, respectively). In total, our data consist of 7244 galaxies at z < 0.5 with precisely measured spectroscopic redshifts, all having impact parameters of 0.01-20 comoving Mpc…

2023 The Astrophysical Journal
eHST 7
Evolution of dynamic fibrils from the cooler chromosphere to the hotter corona
DOI: 10.1051/0004-6361/202347343 Bibcode: 2023A&A...678L...5M

Teriaca, Luca; Solanki, Sami K.; Long, David M. +17 more

Dynamic fibrils (DFs) are commonly observed chromospheric features in solar active regions. Recent observations from the Extreme Ultraviolet Imager (EUI) aboard the Solar Orbiter have revealed unambiguous signatures of DFs at the coronal base in extreme ultraviolet (EUV) emission. However, it remains unclear if the DFs detected in the EUV are link…

2023 Astronomy and Astrophysics
IRIS SolarOrbiter 7
The Great Dimming of the Hypergiant Star RW Cephei: CHARA Array Images and Spectral Analysis
DOI: 10.3847/1538-3881/ace59d Bibcode: 2023AJ....166...78A

Gies, Douglas R.; Monnier, John D.; Schaefer, Gail H. +15 more

The cool hypergiant star RW Cephei is currently in a deep photometric minimum that began several years ago. This event bears a strong similarity to the Great Dimming of the red supergiant Betelgeuse that occurred in 2019-2020. We present the first resolved images of RW Cephei that we obtained with the CHARA Array interferometer. The angular diamet…

2023 The Astronomical Journal
Gaia 7
TOI-1736 and TOI-2141: Two systems including sub-Neptunes around solar analogs revealed by TESS and SOPHIE
DOI: 10.1051/0004-6361/202347744 Bibcode: 2023A&A...680A..84M

Deleuil, M.; Moutou, C.; Winn, J. N. +32 more

Planetary systems around solar analogs inform us about how planets form and evolve in Solar System-like environments. We report the detection and characterization of two planetary systems around the solar analogs TOI-1736 and TOI-2141 using TESS photometry data and spectroscopic data obtained with the SOPHIE instrument on the 1.93 m telescope at t…

2023 Astronomy and Astrophysics
Gaia 7
Benchmarking Gaia DR3 Apsis with the Hyades and Pleiades open clusters
DOI: 10.1051/0004-6361/202346790 Bibcode: 2023A&A...677A.162B

Brandner, Wolfgang; Calissendorff, Per; Kopytova, Taisiya

Context. The Gaia astrophysical parameters inference system (Apsis) provides astrophysical parameter estimates for several to hundreds of millions of stars.
Aims: We aim to benchmark Gaia DR3 Apsis.
Methods: We compiled approximately 1500 bona fide single stars in the Hyades and Pleiades open clusters for validation of PARSEC isochrones,…

2023 Astronomy and Astrophysics
Gaia 7
Revising the properties of low mass eclipsing binary stars using TESS light curves
DOI: 10.1093/mnras/stad519 Bibcode: 2023MNRAS.521.3405J

Maxted, P. F. L.; Southworth, J.; Mancini, L. +1 more

Precise measurements of stellar parameters are required in order to develop our theoretical understanding of stellar structure. These measurements enable errors and uncertainties to be quantified in theoretical models and constrain the physical interpretation of observed phenomena, such as the inflated radii of low-mass stars.

2023 Monthly Notices of the Royal Astronomical Society
Gaia 7
The HERBAL Model: A Hierarchical Errors-in-variables Bayesian Lognormal Hurdle Model for Galactic Globular Cluster Populations
DOI: 10.3847/1538-4357/ace7b7 Bibcode: 2023ApJ...955...22B

Speagle, Joshua S.; Harris, William E.; Eadie, Gwendolyn M. +1 more

Galaxy stellar mass is known to be monotonically related to the size of the galaxy's globular cluster (GC) population for Milky Way sized and larger galaxies. However, the relation becomes ambiguous for dwarf galaxies, where there is some evidence for a downturn in GC population size at low galaxy masses. Smaller dwarfs are increasingly likely to …

2023 The Astrophysical Journal
eHST 7
Quantification of Carbonates, Oxychlorines, and Chlorine Generated by Heterogeneous Electrochemistry Induced by Martian Dust Activity
DOI: 10.1029/2022GL102127 Bibcode: 2023GeoRL..5002127W

Olsen, Kevin S.; Wang, Alian; Jackson, Andrew W. +4 more

Heterogeneous electrochemistry induced by Martian dust activity is an important type of atmosphere-surface interaction that affects geochemical processes at the Martian surface and in the Martian atmosphere. We have experimentally demonstrated that heterogeneous electrochemistry stimulated by mid-strength dust events can decompose common chloride …

2023 Geophysical Research Letters
ExoMars-16 7
Observational Detection of Higher-Order Secular Perturbations in Tight Hierarchical Triple Stars
DOI: 10.3390/universe9110485 Bibcode: 2023Univ....9..485B

Borkovits, Tamás; Mitnyan, Tibor

In this work, we search for observational evidence of higher-order secular perturbations in three eclipsing binaries. These are slightly eccentric binaries, and they form the inner pairs of tight, compact, hierarchical triple star systems. Simultaneously, we analyze the high-precision satellite (Kepler and TESS) light curves; eclipse timing variat…

2023 Universe
Gaia 7