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A Combined Radio Multi-Survey Catalog of Fermi Unassociated Sources
DOI: 10.3847/1538-4357/acaa33 Bibcode: 2023ApJ...943...51B

Schinzel, F. K.; Bruzewski, S.; Taylor, G. B.

Approximately one-third of existing γ-ray sources identified by the Fermi Gamma-Ray Space Telescope are considered to be unassociated, with no known counterpart at other frequencies/wavelengths. These sources have been the subject of intense scrutiny and observational effort during the observatory's mission lifetime, and here we present a method o…

2023 The Astrophysical Journal
Gaia 6
Resolving Galactic-scale Obscuration of X-Ray AGNs at z ≳ 1 with COSMOS-Web
DOI: 10.3847/2041-8213/acdef4 Bibcode: 2023ApJ...951L..41S

Koekemoer, Anton M.; Gillman, Steven; Hirschmann, Michaela +25 more

A large fraction of the accreting supermassive black hole population is shrouded by copious amounts of gas and dust, particularly in the distant (z ≳ 1) universe. While much of the obscuration is attributed to a parsec-scale torus, there is a known contribution from the larger-scale host galaxy. Using JWST/NIRCam imaging from the COSMOS-Web survey…

2023 The Astrophysical Journal
JWST 6
CCD UBV and Gaia DR3 based analysis of NGC 189, NGC 1758 and NGC 7762 open clusters
DOI: 10.1016/j.asr.2023.04.015 Bibcode: 2023AdSpR..72.1454Y

Bilir, Selçuk; Yontan, Talar; Canbay, Remziye +5 more

This paper presents photometric, astrometric, and kinematic analyses of the open clusters NGC 189, NGC 1758 and NGC 7762 based on CCD UBV photometric and Gaia Data Release 3 (DR3) data. According to membership analyses, we identified 32, 57 and 106 most probable member stars with membership probabilities P ⩾ 0.5 in NGC 189, NGC 1758 and NGC 7762, …

2023 Advances in Space Research
Gaia 6
Energy Budget in the Solar Corona
DOI: 10.3847/1538-4357/aceb64 Bibcode: 2023ApJ...954..108T

Telloni, Daniele; Zank, Gary P.; Adhikari, Laxman +34 more

This paper addresses the first direct investigation of the energy budget in the solar corona. Exploiting joint observations of the same coronal plasma by Parker Solar Probe and the Metis coronagraph aboard Solar Orbiter and the conserved equations for mass, magnetic flux, and wave action, we estimate the values of all terms comprising the total en…

2023 The Astrophysical Journal
SolarOrbiter 6
GALFIT-ing AGN Host Galaxies in COSMOS: HST versus Subaru
DOI: 10.3847/1538-4357/ac9400 Bibcode: 2023ApJ...944..137D

Gallagher, Sarah C.; Urry, C. Megan; Barmby, Pauline +3 more

The COSMOS field has been extensively observed by most major telescopes, including Chandra, HST, and Subaru. HST imaging boasts very high spatial resolution and is used extensively in morphological studies of distant galaxies. Subaru provides lower spatial resolution imaging than HST but a substantially wider field of view with greater sensitivity…

2023 The Astrophysical Journal
eHST 6
RNO 54: A Previously Unappreciated FU Ori Star
DOI: 10.3847/2041-8213/ad0be0 Bibcode: 2023ApJ...958L..27H

De, Kishalay; van Roestel, Jan; Hillenbrand, Lynne A. +1 more

We present evidence in support of the hypothesis that the young stellar object RNO 54 is a mature-stage FU Ori type source. The star was first cataloged as a "red nebulous object" in the 1980s but appears to have undergone its outburst prior to the 1890s. Present-day optical and near-infrared spectra are consistent with those of other FU Ori-type …

2023 The Astrophysical Journal
AKARI Gaia 6
Deciphering Faint Gyrosynchrotron Emission from a Coronal Mass Ejection Using Spectropolarimetric Radio Imaging
DOI: 10.3847/1538-4357/acc385 Bibcode: 2023ApJ...950..164K

Mondal, Surajit; Oberoi, Divya; Kansabanik, Devojyoti

Measurements of the plasma parameters of coronal mass ejections (CMEs), particularly the magnetic field and nonthermal electron population entrained in the CME plasma, are crucial to understand their propagation, evolution, and geo-effectiveness. Spectral modeling of gyrosynchrotron (GS) emission from CME plasma has been regarded as one of the mos…

2023 The Astrophysical Journal
SOHO 6
The role of tidal interactions in the formation of slowly rotating early-type stars in young star clusters
DOI: 10.1093/mnras/stad2674 Bibcode: 2023MNRAS.525.5880H

Wang, Li; de Grijs, Richard; Li, Chengyuan +9 more

The split main sequences found in the colour-magnitude diagrams of star clusters younger than ~600 Myr are suggested to be caused by the dichotomy of stellar rotation rates of upper main-sequence stars. Tidal interactions have been suggested as a possible explanation of the dichotomy of the stellar rotation rates. This hypothesis proposes that the…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 6
The SunPy Project: An interoperable ecosystem for solar data analysis
DOI: 10.3389/fspas.2023.1076726 Bibcode: 2023FrASS..1076726B

Ryan, Daniel F.; Ireland, Jack; Hayes, Laura A. +6 more

The SunPy Project is a community of scientists and software developers creating an ecosystem of Python packages for solar physics. The project includes the sunpy core package as well as a set of affiliated packages. The sunpy core package provides general purpose tools to access data from different providers, read image and time series data, and t…

2023 Frontiers in Astronomy and Space Sciences
SolarOrbiter 6
Isochrone fitting of Galactic globular clusters - V. NGC 6397 and NGC 6809 (M55)
DOI: 10.1093/mnras/stad3134 Bibcode: 2023MNRAS.526.5628G

Gontcharov, George A.; Mosenkov, Aleksandr V.; Khovritchev, Maxim Yu +8 more

We fit various colour-magnitude diagrams (CMDs) of the Galactic globular clusters NGC 6397 and NGC 6809 (M55) by isochrones from the Dartmouth Stellar Evolution Database (DSED) and Bag of Stellar Tracks and Isochrones (BaSTI) for α-enhanced [α/Fe] = +0.4. For the CMDs, we use data sets from Hubble Space Telescope, Gaia, Visible and Infrared Survey…

2023 Monthly Notices of the Royal Astronomical Society
Gaia eHST 6