Search Publications

Stellar Characterization and Radius Inflation of Hyades M-dwarf Stars from the APOGEE Survey
DOI: 10.3847/1538-4357/acd4bd Bibcode: 2023ApJ...951...90W

Pascucci, Ilaria; Bizyaev, Dmitry; Pan, Kaike +23 more

We present a spectroscopic analysis of a sample of 48 M-dwarf stars (0.2 M < M < 0.6 M ) from the Hyades open cluster using high-resolution H-band spectra from the Sloan Digital Sky Survey/Apache Point Observatory Galactic Evolution Experiment (APOGEE) survey. Our methodology adopts spectrum synthesis with LTE MARCS …

2023 The Astrophysical Journal
Gaia 9
Irregular Proton Injection to High Energies at Interplanetary Shocks
DOI: 10.3847/2041-8213/ad03f6 Bibcode: 2023ApJ...957L..13T

Wimmer-Schweingruber, Robert F.; Dresing, Nina; Vainio, Rami +8 more

How thermal particles are accelerated to suprathermal energies is an unsolved issue, crucial for many astrophysical systems. We report novel observations of irregular, dispersive enhancements of the suprathermal particle population upstream of a high-Mach-number interplanetary shock. We interpret the observed behavior as irregular "injections" of …

2023 The Astrophysical Journal
SolarOrbiter 9
The Early Light Curve of the Type Ia Supernova 2021hpr in NGC 3147: Progenitor Constraints with the Companion Interaction Model
DOI: 10.3847/1538-4357/acc10c Bibcode: 2023ApJ...949...33L

Wheeler, J. Craig; Im, Myungshin; Kim, Dohyeong +19 more

The progenitor system of Type Ia supernovae (SNe Ia) is expected to be a close binary system consisting of a carbon/oxygen white dwarf (WD) and a nondegenerate star or another WD. Here, we present results from high-cadence monitoring observations of SN 2021hpr in a spiral galaxy, NGC 3147, and constraints on the progenitor system based on its earl…

2023 The Astrophysical Journal
eHST 9
The Polytropic Behavior of Solar Wind Protons as Observed by the Ulysses Spacecraft during Solar Minimum
DOI: 10.3847/1538-4357/acbf33 Bibcode: 2023ApJ...948...22N

Livadiotis, George; Nicolaou, Georgios; McComas, David J.

We analyze proton bulk parameters derived from Ulysses observations and investigate the polytropic behavior of solar wind protons over a wide range of heliocentric distances and latitudes. The large-scale variations of the proton density and temperature over heliocentric distance indicate that plasma protons are governed by subadiabatic processes …

2023 The Astrophysical Journal
Ulysses 9
A Gaia Data Release 3 View on the Tip of the Red Giant Branch Luminosity
DOI: 10.3847/1538-4357/accd69 Bibcode: 2023ApJ...950...83L

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

The tip of the red giant branch (TRGB) is a standard candle that can be used to help refine the determination of the Hubble constant. Gaia Data Release 3 (DR3) provides synthetic photometry constructed from low-resolution BP/RP spectra for Milky Way field stars that can be used to directly calibrate the luminosity of the TRGB in the Johnson-Cousin…

2023 The Astrophysical Journal
Gaia 9
New Velocity Measurements of NGC 5128 Globular Clusters Out to 130 kpc: Outer Halo Kinematics, Substructure, and Dynamics
DOI: 10.3847/1538-4357/acbf43 Bibcode: 2023ApJ...947...34H

Forbes, Duncan A.; Caldwell, Nelson; Strader, Jay +11 more

We present new radial velocity measurements from the Magellan and the Anglo-Australian Telescopes for 175 previously known and 121 newly confirmed globular clusters (GCs) around NGC 5128, the nearest accessible massive early-type galaxy at D = 3.8 Mpc. Remarkably, 28 of these newly confirmed GCs are at projected radii $\gt 50^{\prime} $ (≳54 kpc),…

2023 The Astrophysical Journal
Gaia eHST 9
A Recipe for Unbiased Background Modeling in Deep Wide-field Astronomical Images
DOI: 10.3847/1538-4357/acdee3 Bibcode: 2023ApJ...953....7L

van Dokkum, Pieter; Abraham, Roberto; Pasha, Imad +9 more

Unbiased sky background modeling is crucial for the analysis of deep wide-field images, but it remains a major challenge in low surface brightness astronomy. Traditional image processing algorithms are often designed to produce artificially flat backgrounds, erasing astrophysically meaningful structures. In this paper, we present three ideas that …

2023 The Astrophysical Journal
Herschel 9
Crossing the Rubicon of Reionization with z 5 QSOs
DOI: 10.3847/1538-4357/aceb60 Bibcode: 2023ApJ...955...60G

Grazian, Andrea; Boutsia, Konstantina; Fiore, Fabrizio +12 more

One of the key open questions in cosmology is the nature of sources that completed cosmological hydrogen reionization at z ~ 5.2. High-z primeval galaxies have been long considered the main drivers of reionization, with a minor role played by high-z active galactic nuclei (AGN). However, in order to confirm this scenario, it is fundamental to meas…

2023 The Astrophysical Journal
Gaia 9
Lack of Correlations between Cold Molecular Gas and AGN Properties in Type 1 AGNs at z ≲ 0.5
DOI: 10.3847/1538-4357/acc9b4 Bibcode: 2023ApJ...950...60M

Ho, Luis C.; Bauer, Franz E.; Treister, Ezequiel +3 more

We present new NOrthern Extended Millimeter Array (NOEMA) observations of the CO(2-1) emission in eight of the brightest Palomar-Green quasars at z ≲ 0.5 to investigate the role of active galactic nucleus (AGN) feedback in luminous quasars detected at low redshifts. We detect CO(2-1) emission in three objects, from which we derive CO luminosities,…

2023 The Astrophysical Journal
Herschel 9
A Multiwavelength Light-curve Analysis of the Classical Nova YZ Ret: An Extension of the Universal Decline Law to the Nebular Phase
DOI: 10.3847/1538-4357/acdfd3 Bibcode: 2023ApJ...953...78H

Kato, Mariko; Hachisu, Izumi

YZ Ret is the first X-ray flash detected classical nova, and is also observed in optical, X-ray, and gamma-ray. We propose a comprehensive model that explains the observational properties. The white dwarf mass is determined to be ~1.33 M , which reproduces the multiwavelength light curves of YZ Ret, from optical, X-ray, to gamma-ray. W…

2023 The Astrophysical Journal
Gaia XMM-Newton 9