Search Publications

The Role of High-frequency Transverse Oscillations in Coronal Heating
DOI: 10.3847/2041-8213/ace423 Bibcode: 2023ApJ...952L..15L

Van Doorsselaere, Tom; Lim, Daye; Berghmans, David +3 more

Transverse oscillations that do not show significant damping in solar coronal loops are found to be ubiquitous. Recently, the discovery of high-frequency transverse oscillations in small-scale loops has been accelerated by the Extreme Ultraviolet Imager on board Solar Orbiter. We perform a meta-analysis by considering the oscillation parameters re…

2023 The Astrophysical Journal
SolarOrbiter 20
Magnetic Field Spectral Evolution in the Inner Heliosphere
DOI: 10.3847/2041-8213/acaeff Bibcode: 2023ApJ...943L...8S

Fedorov, A.; Horbury, T. S.; Louarn, P. +24 more

Parker Solar Probe and Solar Orbiter data are used to investigate the radial evolution of magnetic turbulence between 0.06 ≲ R ≲ 1 au. The spectrum is studied as a function of scale, normalized to the ion inertial scale d i . In the vicinity of the Sun, the inertial range is limited to a narrow range of scales and exhibits a power-law …

2023 The Astrophysical Journal
SolarOrbiter 20
PHANGS-JWST First Results: Stellar-feedback-driven Excitation and Dissociation of Molecular Gas in the Starburst Ring of NGC 1365?
DOI: 10.3847/2041-8213/aca973 Bibcode: 2023ApJ...944L..19L

Bolatto, Alberto D.; Henshaw, Jonathan D.; Kruijssen, J. M. Diederik +36 more

We compare embedded young massive star clusters (YMCs) to (sub-)millimeter line observations tracing the excitation and dissociation of molecular gas in the starburst ring of NGC 1365. This galaxy hosts one of the strongest nuclear starbursts and richest populations of YMCs within 20 Mpc. Here we combine near-/mid-IR PHANGS-JWST imaging with new A…

2023 The Astrophysical Journal
eHST JWST 20
The Bimodal Absorption System Imaging Campaign (BASIC). I. A Dual Population of Low-metallicity Absorbers at z < 1
DOI: 10.3847/1538-4357/acb047 Bibcode: 2023ApJ...944..101B

Johnson, Sean D.; Tripp, Todd M.; Prochaska, J. Xavier +17 more

The bimodal absorption system imaging campaign (BASIC) aims to characterize the galaxy environments of a sample of 36 H I-selected partial Lyman limit systems (pLLSs) and Lyman limit systems (LLSs) in 23 QSO fields at z ≲ 1. These pLLSs/LLSs provide a unique sample of absorbers with unbiased and well-constrained metallicities, allowing us to explo…

2023 The Astrophysical Journal
eHST 20
A Hydrodynamic Study of the Escape of Metal Species and Excited Hydrogen from the Atmosphere of the Hot Jupiter WASP-121b
DOI: 10.3847/1538-4357/accd5e Bibcode: 2023ApJ...951..123H

Lavvas, Panayotis; Koskinen, Tommi; Fossati, Luca +1 more

In the near-UV and optical transmission spectrum of the hot Jupiter WASP-121b, recent observations have detected strong absorption features of Mg, Fe, Ca, and Hα, extending outside of the planet's Roche lobe. Studying these atomic signatures can directly trace the escaping atmosphere and constrain the energy balance of the upper atmosphere. To und…

2023 The Astrophysical Journal
eHST 20
JWST Measurements of 13C, 18O, and 17O in the Atmosphere of Super-Jupiter VHS 1256 b
DOI: 10.3847/2041-8213/ad07e2 Bibcode: 2023ApJ...957L..36G

Zhang, Yapeng; Gandhi, Siddharth; de Regt, Sam +4 more

Isotope ratios have recently been measured in the atmospheres of directly imaged and transiting exoplanets from ground-based observations. The arrival of JWST allows us to characterize exoplanetary atmospheres in further detail and opens up wavelengths inaccessible from the ground. In this work we constrain the carbon and oxygen isotopes 13

2023 The Astrophysical Journal
JWST 20
Weak-lensing Mass Bias in Merging Galaxy Clusters
DOI: 10.3847/1538-4357/acb76b Bibcode: 2023ApJ...945...71L

Nagai, Daisuke; Jee, M. James; Finner, Kyle +6 more

Although weak lensing (WL) is a powerful method to estimate a galaxy cluster mass without any dynamical assumptions, a model bias can arise when the cluster density profile departs from the assumed model profile. In a merging system, the bias is expected to become most severe because the constituent halos undergo significant structural changes. In…

2023 The Astrophysical Journal
eHST 20
Confirmation of an Anomalously Low Dark Matter Content for the Galaxy NGC 1052-DF4 from Deep, High-resolution Continuum Spectroscopy
DOI: 10.3847/1538-4357/acfa70 Bibcode: 2023ApJ...957....6S

van Dokkum, Pieter; Shen, Zili; Danieli, Shany

NGC 1052-DF4 was found to be the second "galaxy lacking dark matter" in the NGC 1052 group, based on its velocity dispersion of ${\sigma }_{\mathrm{gc}}={4.2}_{-2.2}^{+4.4}$ km s-1 as measured from the radial velocities of seven of its globular clusters. Here we verify this result by measuring the stellar velocity dispersion of the gala…

2023 The Astrophysical Journal
eHST 20
The ELM Survey South. II. Two Dozen New Low-mass White Dwarf Binaries
DOI: 10.3847/1538-4357/acd187 Bibcode: 2023ApJ...950..141K

Gianninas, A.; Kupfer, Thomas; Kilic, Mukremin +5 more

We present the results from our ongoing spectroscopic survey targeting low-mass white dwarf binaries, focusing on the southern sky. We used a Gaia DR2- and eDR3-based selection and identified 28 new binaries, including 19 new extremely low-mass (ELM) white dwarfs, one short period, likely eclipsing, DABZ, and two potential LISA binaries. We presen…

2023 The Astrophysical Journal
Gaia 20
SPLUS J142445.34-254247.1: An r-process-enhanced, Actinide-boost, Extremely Metal-poor Star Observed with GHOST
DOI: 10.3847/1538-4357/ad077e Bibcode: 2023ApJ...959...60P

Jones, David O.; Simpson, Chris; Placco, Vinicius M. +33 more

We report on a chemo-dynamical analysis of SPLUS J142445.34-254247.1 (SPLUS J1424-2542), an extremely metal-poor halo star enhanced in elements formed by the rapid neutron-capture process (r-process). This star was first selected as a metal-poor candidate from its narrowband S-PLUS photometry and followed up spectroscopically in medium resolution …

2023 The Astrophysical Journal
Gaia 20