Search Publications

Luminous Supernovae: Unveiling a Population between Superluminous and Normal Core-collapse Supernovae
DOI: 10.3847/1538-4357/ac9842 Bibcode: 2022ApJ...941..107G

Berger, Edo; Nicholl, Matt; Hosseinzadeh, Griffin +2 more

Stripped-envelope core-collapse supernovae can be divided into two broad classes: the common Type Ib/c supernovae (SNe Ib/c), powered by the radioactive decay of 56Ni, and the rare superluminous supernovae (SLSNe), most likely powered by the spin-down of a magnetar central engine. Up to now, the intermediate regime between these two pop…

2022 The Astrophysical Journal
Gaia 44
Luminous Millimeter, Radio, and X-Ray Emission from ZTF 20acigmel (AT 2020xnd)
DOI: 10.3847/1538-4357/ac4e97 Bibcode: 2022ApJ...932..116H

Kaplan, David L.; Petitpas, Glen; Perley, Daniel A. +7 more

Observations of the extragalactic (z = 0.0141) transient AT 2018cow established a new class of energetic explosions shocking a dense medium, producing luminous emission at millimeter and submillimeter wavelengths. Here we present detailed millimeter- through centimeter-wave observations of a similar transient, ZTF 20acigmel (AT 2020xnd), at z = 0.…

2022 The Astrophysical Journal
Gaia 44
ALMA Reveals Extended Cool Gas and Hot Ionized Outflows in a Typical Star-forming Galaxy at Z = 7.13
DOI: 10.3847/1538-4357/ac795b Bibcode: 2022ApJ...934...64A

Richard, Johan; Fujimoto, Seiji; Inoue, Akio K. +9 more

We present spatially resolved morphological properties of [C II] 158 µm, [O III] 88 µm, dust, and rest-frame ultraviolet (UV) continuum emission for A1689-zD1, a strongly lensed, sub-L* galaxy at z = 7.13, by utilizing deep Atacama Large Millimeter/submillimeter Array (ALMA) and Hubble Space Telescope (HST) observations. While the [O I…

2022 The Astrophysical Journal
eHST 44
Probing the Physics of the Solar Atmosphere with the Multi-slit Solar Explorer (MUSE). II. Flares and Eruptions
DOI: 10.3847/1538-4357/ac4223 Bibcode: 2022ApJ...926...53C

Reeves, Katharine K.; Polito, Vanessa; Golub, Leon +25 more

Current state-of-the-art spectrographs cannot resolve the fundamental spatial (subarcseconds) and temporal (less than a few tens of seconds) scales of the coronal dynamics of solar flares and eruptive phenomena. The highest-resolution coronal data to date are based on imaging, which is blind to many of the processes that drive coronal energetics a…

2022 The Astrophysical Journal
IRIS 44
The VLA/ALMA Nascent Disk And Multiplicity (VANDAM) Survey of Orion Protostars. V. A Characterization of Protostellar Multiplicity
DOI: 10.3847/1538-4357/ac36d2 Bibcode: 2022ApJ...925...39T

Kratter, Kaitlin M.; Li, Zhi-Yun; van Dishoeck, Ewine F. +16 more

We characterize protostellar multiplicity in 20 Current address: Niels Bohr Institute, University of Copenhagen, Øster Voldgade 5–7, DK-1350, Copenhagen K, Denmark. the Orion molecular clouds using Atacama Large Millimeter/submillimeter Array 0.87 mm and Very Large Array 9 mm continuum surveys toward 328 protostars. These observations…

2022 The Astrophysical Journal
eHST 43
The Atari Disk, a Metal-poor Stellar Population in the Disk System of the Milky Way
DOI: 10.3847/1538-4357/ac8102 Bibcode: 2022ApJ...936...78M

Frebel, Anna; Mardini, Mohammad K.; Chiti, Anirudh +3 more

We have developed a chemodynamical approach to assign 36,010 metal-poor SkyMapper stars to various Galactic stellar populations. Using two independent techniques (velocity and action space behavior), Gaia EDR3 astrometry, and photometric metallicities, we selected stars with the characteristics of the "metal-weak" thick-disk population by minimizi…

2022 The Astrophysical Journal
Gaia 43
New Roads to the Small-scale Universe: Measurements of the Clustering of Matter with the High-redshift UV Galaxy Luminosity Function
DOI: 10.3847/2041-8213/ac5e9c Bibcode: 2022ApJ...928L..20S

Muñoz, Julian B.; Sabti, Nashwan; Blas, Diego

The epochs of cosmic dawn and reionization present promising avenues for understanding the role of dark matter (DM) in our cosmos. The first galaxies that populated the universe during these eras resided in DM halos that were much less massive than their counterparts today. Consequently, observations of such galaxies can provide us with a handle o…

2022 The Astrophysical Journal
eHST 43
Exploring the Sgr-Milky Way-disk Interaction Using High-resolution N-body Simulations
DOI: 10.3847/1538-4357/ac5021 Bibcode: 2022ApJ...927..131B

Bovy, Jo; Hunt, Jason A. S.; Bennett, Morgan

The ongoing merger of the Sagittarius (Sgr) dwarf galaxy with the Milky Way is believed to strongly affect the dynamics of the Milky Way's disk. We present a suite of 13 N-body simulations, with 500 million-1 billion particles, modeling the interaction between the Sgr dwarf galaxy and the Galactic disk. To quantify the perturbation to the disk's s…

2022 The Astrophysical Journal
Gaia 42
The Mass of the Milky Way from the H3 Survey
DOI: 10.3847/1538-4357/ac3a7a Bibcode: 2022ApJ...925....1S

Conroy, Charlie; Ting, Yuan-Sen; Cargile, Phillip A. +8 more

The mass of the Milky Way is a critical quantity that, despite decades of research, remains uncertain within a factor of two. Until recently, most studies have used dynamical tracers in the inner regions of the halo, relying on extrapolations to estimate the mass of the Milky Way. In this paper, we extend the hierarchical Bayesian model applied in…

2022 The Astrophysical Journal
Gaia 42
The Tidal Disruption Event AT2021ehb: Evidence of Relativistic Disk Reflection, and Rapid Evolution of the Disk-Corona System
DOI: 10.3847/1538-4357/ac898a Bibcode: 2022ApJ...937....8Y

Kulkarni, S. R.; Sunyaev, R.; Cenko, S. Bradley +29 more

We present X-ray, UV, optical, and radio observations of the nearby (≈78 Mpc) tidal disruption event AT2021ehb/ZTF21aanxhjv during its first 430 days of evolution. AT2021ehb occurs in the nucleus of a galaxy hosting a≈107 M black hole (M BH inferred from host galaxy scaling relations). High-cadence Swift and Neut…

2022 The Astrophysical Journal
XMM-Newton 42