Search Publications

The Stellar Mass Function in CANDELS and Frontier Fields: The Buildup of Low-mass Passive Galaxies since z 3
DOI: 10.3847/1538-4357/ac9a48 Bibcode: 2022ApJ...940..135S

Santini, Paola; Calabrò, Antonello; Castellano, Marco +8 more

Despite significant efforts in recent years, the physical processes responsible for the formation of passive galaxies through cosmic time remain unclear. The shape and evolution of the stellar mass function (SMF) give an insight into these mechanisms. Taking advantage of the CANDELS and the deep Hubble Frontier Fields (HFF) programs, we estimated …

2022 The Astrophysical Journal
eHST 25
Monochromatic Globular Clusters as a Critical Test of Formation Models for the Dark Matter-deficient Galaxies NGC 1052-DF2 and NGC 1052-DF4
DOI: 10.3847/2041-8213/ac94d6 Bibcode: 2022ApJ...940L...9V

van Dokkum, Pieter; Romanowsky, Aaron J.; Conroy, Charlie +8 more

It was recently proposed that the dark matter-deficient ultradiffuse galaxies DF2 and DF4 in the NGC 1052 group could be the products of a "bullet dwarf" collision between two gas-rich progenitor galaxies. In this model, DF2 and DF4 formed at the same time in the immediate aftermath of the collision, and a strong prediction is that their globular …

2022 The Astrophysical Journal
eHST 25
LoTSS Jellyfish Galaxies. IV. Enhanced Star Formation on the Leading Half of Cluster Galaxies and Gas Compression in IC3949
DOI: 10.3847/1538-4357/ac9e9f Bibcode: 2022ApJ...941...77R

Ellison, Sara L.; Lin, Lihwai; Pan, Hsi-An +7 more

With Mapping Nearby Galaxies at APO integral field spectroscopy, we present a resolved analysis of star formation for 29 jellyfish galaxies in nearby clusters, identified from radio continuum imaging taken by the Low Frequency Array. Simulations predict enhanced star formation on the "leading half" (LH) of galaxies undergoing ram pressure strippin…

2022 The Astrophysical Journal
eHST 24
Role of Magnetic Fields in Fueling Seyfert Nuclei
DOI: 10.3847/1538-4357/ac9df0 Bibcode: 2022ApJ...941...92H

Beck, Rainer; Lazarian, A.; Hu, Yue +1 more

Molecular gas is believed to be the fuel for star formation and nuclear activity in Seyfert galaxies. To explore the role of magnetic fields in funneling molecular gas into the nuclear region, measurements of the magnetic fields embedded in molecular gas are needed. By applying the new velocity gradient technique (VGT) to CO isotopolog data from t…

2022 The Astrophysical Journal
eHST 24
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