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Hubble Space Telescope Observations of GW170817: Complete Light Curves and the Properties of the Galaxy Merger of NGC 4993
DOI: 10.3847/1538-4357/ac3e59 Bibcode: 2022ApJ...926...49K

Kilpatrick, Charles D.; Leja, Joel; Fong, Wen-fai +10 more

We present the complete set of Hubble Space Telescope imaging of the binary neutron star merger GW170817 and its optical counterpart AT 2017gfo. Including deep template imaging in F814W, F110W, F140W, and F160W at 3.4 yr post-merger, we reanalyze the full light curve of AT 2017gfo across 12 bands from 5 to 1273 rest-frame days after merger. We obt…

2022 The Astrophysical Journal
eHST 24
Properties of Host Galaxies of Submillimeter Sources as Revealed by JWST Early Release Observations in SMACS J0723.3-7327
DOI: 10.3847/2041-8213/ac8d08 Bibcode: 2022ApJ...936L..19C

Yan, Haojing; Cheng, Cheng; Willmer, Christopher N. A. +3 more

Using the 0.9-4.4 µm imaging data from the James Webb Space Telescope (JWST) early release observation in the SMACS J0723.3-7327 galaxy cluster field, we discuss the properties of three submillimeter galaxies (SMGs) detected by the Atacama Large Millimeter/submillimeter Array Array. These sources are magnified by 1.4-2.1 × due to gravitation…

2022 The Astrophysical Journal
eHST JWST 24
Patches of Magnetic Switchbacks and Their Origins
DOI: 10.3847/1538-4357/ac7c11 Bibcode: 2022ApJ...934..152S

de Wit, Thierry Dudok; Velli, Marco; Bale, Stuart D. +18 more

Parker Solar Probe (PSP) has shown that the solar wind in the inner heliosphere is characterized by the quasi omnipresence of magnetic switchbacks ("switchback" hereinafter), local backward bends of magnetic field lines. Switchbacks also tend to come in patches, with a large-scale modulation that appears to have a spatial scale size comparable to …

2022 The Astrophysical Journal
Hinode 24
A Maximum Likelihood Calibration of the Tip of the Red Giant Branch Luminosity from High Latitude Field Giants Using Gaia Early Data Release 3 Parallaxes
DOI: 10.3847/1538-4357/ac7559 Bibcode: 2022ApJ...939...96L

Casertano, Stefano; Li, Siyang; Riess, Adam G.

The calibration of the tip of the red giant branch (TRGB) in the I band has a direct role in determinations of the Hubble constant, a subject of recent interest due to the discrepancy between direct and indirect estimates of its value. We present a maximum likelihood method designed to obtain an independent calibration of the brightness of TRGB us…

2022 The Astrophysical Journal
Gaia 24
Luminosities and Masses of Single Galactic Post-asymptotic Giant Branch Stars with Distances from Gaia EDR3: The Revelation of an s-process Diversity
DOI: 10.3847/2041-8213/ac5686 Bibcode: 2022ApJ...927L..13K

Ventura, Paolo; Van Winckel, Hans; Hrivnak, Bruce J. +4 more

Post-asymptotic giant branch (AGB) stars are exquisite probes of AGB nucleosynthesis. However, the previous lack of accurate distances jeopardized comparison with theoretical AGB models. The Gaia Early Data Release 3 (Gaia EDR3) has now allowed for a breakthrough in this research landscape. In this study, we focus on a sample of single Galactic po…

2022 The Astrophysical Journal
Gaia 24
Intrinsic Lyα Profiles of High-velocity G, K, and M Dwarfs
DOI: 10.3847/1538-4357/ac4711 Bibcode: 2022ApJ...926..129Y

Redfield, Seth; France, Kevin; Youngblood, Allison +5 more

Observations of H I Lyman α, the brightest UV emission line of late-type stars, are critical for understanding stellar chromospheres and transition regions, modeling photochemistry in exoplanet atmospheres, and measuring the abundances of neutral hydrogen and deuterium in the interstellar medium. Yet Lyα observations are notoriously challenging ow…

2022 The Astrophysical Journal
Gaia IRIS SOHO eHST 24
Survey of Multiple Populations in Globular Clusters among Very-low-mass Stars
DOI: 10.3847/1538-4357/ac5046 Bibcode: 2022ApJ...927..207D

Milone, A. P.; Cordoni, G.; Marino, A. F. +14 more

Recent work has shown that near-infrared (NIR) Hubble Space Telescope (HST) photometry allows us to disentangle multiple populations (MPs) among M dwarfs of globular clusters (GCs) and to investigate this phenomenon in very-low-mass (VLM) stars. Here, we present the color-magnitude diagrams of nine GCs and the open cluster NGC 6791 in the F110W an…

2022 The Astrophysical Journal
eHST 24
Constraining the Nature of the 18 min Periodic Radio Transient GLEAM-X J162759.5-523504.3 via Multiwavelength Observations and Magneto-thermal Simulations
DOI: 10.3847/1538-4357/ac97ea Bibcode: 2022ApJ...940...72R

de Martino, D.; Rea, N.; Buckley, D. A. H. +14 more

We observed the periodic radio transient GLEAM-X J162759.5-523504.3 (GLEAM-X J1627) using the Chandra X-ray Observatory for about 30 ks on 2022 January 22-23, simultaneously with radio observations from the Murchison Widefield Array, MeerKAT, and the Australia Telescope Compact Array. Its radio emission and 18 min periodicity led the source to be …

2022 The Astrophysical Journal
Gaia 24
The Panchromatic Hubble Andromeda Treasury: Triangulum Extended Region (PHATTER). II. The Spatially Resolved Recent Star Formation History of M33
DOI: 10.3847/1538-4357/ac7568 Bibcode: 2022ApJ...934...76L

Bell, Eric F.; Williams, Benjamin F.; Choi, Yumi +11 more

We measure the spatially resolved recent star formation history (SFH) of M33 using optical images taken with the Hubble Space Telescope as part of the Panchromatic Hubble Andromeda Treasury: Triangulum Extended Region (PHATTER) survey. The area covered by the observations used in this analysis covers a de-projected area of ~38 kpc2 and …

2022 The Astrophysical Journal
eHST 24
A New Magnetic Parameter of Active Regions Distinguishing Large Eruptive and Confined Solar Flares
DOI: 10.3847/2041-8213/ac5251 Bibcode: 2022ApJ...926L..14L

Hou, Yijun; Li, Ting; Yang, Shuhong +3 more

With the aim of investigating how the magnetic field in solar active regions (ARs) controls flare activity, i.e., whether a confined or eruptive flare occurs, we analyze 106 flares of Geostationary Operational Environmental Satellite class ≥M1.0 during 2010-2019. We calculate mean characteristic twist parameters α FPIL within the "flari…

2022 The Astrophysical Journal
SOHO 24