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Observational Evidence of S-web Source of the Slow Solar Wind
DOI: 10.3847/1538-4357/acc653 Bibcode: 2023ApJ...950...65B

Barczynski, K.; Peter, H.; Zhukov, A. N. +25 more

From 2022 March 18 to 21, NOAA Active Region (AR) 12967 was tracked simultaneously by Solar Orbiter at 0.35 au and Hinode/EIS at Earth. During this period, strong blueshifted plasma upflows were observed along a thin, dark corridor of open magnetic field originating at the AR's leading polarity and continuing toward the southern extension of the n…

2023 The Astrophysical Journal
Hinode SolarOrbiter 20
CLEAR: Survey Overview, Data Analysis, and Products
DOI: 10.3847/1538-4365/acc517 Bibcode: 2023ApJS..266...13S

Papovich, Casey; Finkelstein, Steven L.; Cleri, Nikko J. +19 more

We present an overview of the CANDELS Lyα Emission At Reionization (CLEAR) survey. CLEAR is a 130 orbit program of the Hubble Space Telescope using the Wide Field Camera 3 (WFC3) IR G102 grism. CLEAR targets 12 pointings divided between the GOODS-N and GOODS-S fields of the Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey (CANDELS). Combin…

2023 The Astrophysical Journal Supplement Series
eHST 20
New compact hierarchical triple system candidates identified using Gaia DR3
DOI: 10.1051/0004-6361/202245300 Bibcode: 2023A&A...670A..75C

Mitnyan, T.; Pál, A.; Borkovits, T. +5 more


Aims: We introduce a novel way to identify new compact hierarchical triple stars by exploiting the huge potential of Gaia DR3 and also its future data releases. We aim to increase the current number of compact hierarchical triple systems significantly.
Methods: We used several eclipsing binary catalogs from different sky surveys that lis…

2023 Astronomy and Astrophysics
Gaia 20
JWST Peers into the Class I Protostar TMC1A: Atomic Jet and Spatially Resolved Dissociative Shock Region
DOI: 10.3847/2041-8213/acdfca Bibcode: 2023ApJ...951L..32H

Pontoppidan, K. M.; Bjerkeli, P.; Kristensen, L. E. +6 more

Outflows and winds launched from young stars play a crucial role in the evolution of protostars and the early stages of planet formation. However, the specific details of the mechanism behind these phenomena, including how they affect the protoplanetary disk structure, are still debated. We present JWST NIRSpec integral field unit observations of …

2023 The Astrophysical Journal
Herschel eHST JWST 20
Giant Planet Engulfment by Evolved Giant Stars: Light Curves, Asteroseismology, and Survivability
DOI: 10.3847/1538-4357/acd2d4 Bibcode: 2023ApJ...950..128O

Bildsten, Lars; Cantiello, Matteo; O'Connor, Christopher E. +1 more

About ten percent of Sun-like (1-2 M ) stars will engulf a 1-10 M J planet as they expand during the red giant branch (RGB) or asymptotic giant branch (AGB) phase of their evolution. Once engulfed, these planets experience a strong drag force in the star's convective envelope and spiral inward, depositing energy and angular …

2023 The Astrophysical Journal
Gaia 20
The radio emission in radio-quiet quasars: the VLBA perspective
DOI: 10.1093/mnras/stad2289 Bibcode: 2023MNRAS.525..164C

Gelfand, Joseph D.; Laor, Ari; Behar, Ehud +2 more

The origin of the radio emission in radio-quiet quasars (RQQ) is not established yet. We present new VLBA observations at 1.6 and 4.9 GHz of 10 RQQ (9 detected), which together with published earlier observations of 8 RQQ (5 detected), forms a representative sample of 18 RQQ drawn from the Palomar-Green sample of low z (< 0.5) AGN. The spectral…

2023 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 20
Exoplanet spectroscopy with JWST NIRISS: diagnostics and case studies
DOI: 10.1093/mnras/stad1580 Bibcode: 2023MNRAS.524..377H

Madhusudhan, Nikku; Holmberg, Måns

The JWST is ushering in a new era in remote sensing of exoplanetary atmospheres. Atmospheric retrievals of exoplanets can be highly sensitive to high-precision JWST data. It is, therefore, imperative to characterize the instruments and noise sources using early observations to enable robust characterization of exoplanetary atmospheres using JWST-q…

2023 Monthly Notices of the Royal Astronomical Society
Gaia JWST 20
Cosmic Evolution of Gas and Star Formation
DOI: 10.3847/1538-4357/aca1bc Bibcode: 2023ApJ...943...82S

Staguhn, Johannes; Mobasher, Bahram; Capak, Peter +20 more

Atacama Large Millimeter/submillimeter Array (ALMA) observations of the long-wavelength dust continuum are used to estimate the gas masses in a sample of 708 star-forming galaxies at z = 0.3-4.5. We determine the dependence of gas masses and star formation efficiencies (SFEs; SFR per unit gas mass) on redshift (z), M *, and star formati…

2023 The Astrophysical Journal
Herschel 20
Observable Signatures of Stellar-mass Black Holes in Active Galactic Nuclei
DOI: 10.3847/2041-8213/acc103 Bibcode: 2023ApJ...946L...3T

Perna, Rosalba; Tagawa, Hiromichi; Kimura, Shigeo S. +2 more

Stellar-mass black holes (BHs) are predicted to be embedded in the disks of active galactic nuclei (AGNs) due to gravitational drag and in situ star formation. However, clear evidence for AGN disk-embedded BHs is currently lacking. Here, as possible electromagnetic signatures of these BHs, we investigate breakout emission from shocks emerging arou…

2023 The Astrophysical Journal
XMM-Newton 20
The Planck clusters in the LOFAR sky. III. LoTSS-DR2: Dynamic states and density fluctuations of the intracluster medium
DOI: 10.1051/0004-6361/202244761 Bibcode: 2023A&A...672A..42Z

Simionescu, A.; Kaastra, J. S.; Zhang, X. +19 more

Context. The footprint of the recent second data release of the LOFAR Two-metre Sky Survey (LoTSS-DR2) covers 309 Planck Sunyaev-Zeldovich (SZ) selected galaxy clusters, 83 of which host a radio halo and 26 host a radio relic(s). It provides an excellent opportunity to statistically study the properties of extended cluster radio sources, especiall…

2023 Astronomy and Astrophysics
XMM-Newton 20