Search Publications

Mixed Modes and Asteroseismic Surface Effects. II. Subgiant Systematics
DOI: 10.3847/1538-4357/ac1e8b Bibcode: 2021ApJ...922...18O

Bieryla, Allyson; Latham, David W.; Basu, Sarbani +3 more

Models of solar-like oscillators yield acoustic modes at different frequencies than would be seen in actual stars possessing identical interior structure, due to modeling error near the surface. This asteroseismic "surface term" must be corrected when mode frequencies are used to infer stellar structure. Subgiants exhibit oscillations of mixed aco…

2021 The Astrophysical Journal
Gaia 13
A Distance-deviation Consistency and Model-independent Method to Test the Cosmic Distance-Duality Relation
DOI: 10.3847/1538-4357/abc9bf Bibcode: 2021ApJ...909..118Z

Fang, Guanwen; Zhou, Chichun; Hu, Jian +2 more

A distance-deviation consistency and model-independent method to test the cosmic distance-duality relation (CDDR) is provided. This method is worthy of attention for two reasons. First, a distance-deviation consistency method is used to pair subsamples: instead of pairing subsamples with redshift deviations smaller than a value of, say, $\left|{\r…

2021 The Astrophysical Journal
eHST 13
Kinetic Alfvén Waves in Space Plasma Environment with κ-electrons
DOI: 10.3847/1538-4357/ac0c1f Bibcode: 2021ApJ...919...71B

Lakhina, G. S.; Singh, S. V.; Barik, K. C.

A resonant instability of kinetic Alfvén waves (KAWs) driven by ion beam is discussed through a theoretical model encompassing Maxwellian background ions and beam ions and non-Maxwellian κ-electrons. The ion beam velocity alone as a source is able to excite the KAWs up to a significant growth. The non-Maxwellian parameter κ impedes the growth of K…

2021 The Astrophysical Journal
Cluster 13
Resolved Nuclear Kinematics Link the Formation and Growth of Nuclear Star Clusters with the Evolution of Their Early- and Late-type Hosts
DOI: 10.3847/1538-4357/ac158f Bibcode: 2021ApJ...921....8P

Böker, Torsten; Neumayer, Nadine; Emsellem, Eric +7 more

We present parsec-scale kinematics of 11 nearby galactic nuclei, derived from adaptive-optics assisted integral-field spectroscopy at (near-infrared) CO band-head wavelengths. We focus our analysis on the balance between ordered rotation and random motions, which can provide insights into the dominant formation mechanism of nuclear star clusters (…

2021 The Astrophysical Journal
eHST 12
Electron Densities in the Solar Corona Measured Simultaneously in the Extreme Ultraviolet and Infrared
DOI: 10.3847/1538-4357/abcd91 Bibcode: 2021ApJ...906..118D

Del Zanna, Giulio; Dudík, Jaroslav; Dzifčáková, Elena +5 more

Accurate measurements of electron density are critical for determination of the plasma properties in the solar corona. We compare the electron densities diagnosed from Fe XIII lines observed by the Extreme-Ultraviolet Imaging Spectrometer (EIS) onboard the Hinode mission with the near-infrared (NIR) measurements provided by the ground-based Corona…

2021 The Astrophysical Journal
Hinode 12
The Center of Expansion and Age of the Oxygen-rich Supernova Remnant 1E 0102.2-7219
DOI: 10.3847/1538-4357/abe2a7 Bibcode: 2021ApJ...912...33B

Drout, Maria R.; Blair, William P.; Margutti, Raffaella +8 more

We present new proper-motion measurements of optically emitting oxygen-rich knots of supernova remnant 1E 0102.2-7219 (E0102), which are used to estimate the remnant's center of expansion and age. Four epochs of high-resolution Hubble Space Telescope images spanning 19 yr were retrieved and analyzed. We found a robust center of expansion of α = 1<…

2021 The Astrophysical Journal
eHST 12
Analysis of the Unconcentrated Background of the EPIC pn Camera on Board XMM-Newton
DOI: 10.3847/1538-4357/abcfbc Bibcode: 2021ApJ...908...37M

Esposito, Paolo; Tiengo, Andrea; De Luca, Andrea +8 more

Our understanding of the background of the EPIC/pn camera on board XMM-Newton is incomplete. This affects the study of extended sources and can influence the predictions of the expected background of future X-ray missions, such as the Advanced Telescope for High Energy Astrophysics (ATHENA). Here we provide new results based on the analysis of the…

2021 The Astrophysical Journal
INTEGRAL XMM-Newton 12
Acceleration of Ring Current Protons Driven by Magnetosonic Waves: Comparisons of Test Particle Simulations with Quasilinear Calculations
DOI: 10.3847/1538-4357/abd2b3 Bibcode: 2021ApJ...908..203F

Fu, Song; Ge, Yasong

Wave-particle interactions play important roles in local acceleration and pitch angle scattering loss of charged particle dynamics in astrophysics and space physics, and energy transfer between plasma waves and particles is a key problem in plasma physics. Using full relativistic test particle simulations, we quantitatively evaluate the magnetoson…

2021 The Astrophysical Journal
Cluster 12
Star Formation Histories from Spectral Energy Distributions and Color-magnitude Diagrams Agree: Evidence for Synchronized Star Formation in Local Volume Dwarf Galaxies over the Past 3 Gyr
DOI: 10.3847/1538-4357/abf3c2 Bibcode: 2021ApJ...913...45O

McQuinn, Kristen B. W.; Johnson, Benjamin D.; Gawiser, Eric +6 more

Star formation histories (SFHs) reveal physical processes that influence how galaxies form their stellar mass. We compare the SFHs of a sample of 36 nearby (D ⪅ 4 Mpc) dwarf galaxies from the ACS Nearby Galaxy Survey Treasury (ANGST), inferred from the color-magnitude diagrams (CMDs) of individually resolved stars in these galaxies, with those rec…

2021 The Astrophysical Journal
eHST 12
Blow-away in the Extreme Low-mass Starburst Galaxy Pox 186
DOI: 10.3847/1538-4357/abe85d Bibcode: 2021ApJ...912...12E

Scarlata, Claudia; Jaskot, Anne; Skillman, Evan +1 more

Pox 186 is an exceptionally small dwarf starburst galaxy hosting a stellar mass of ∼105 M. Undetected in H I (M < 106 M) from deep 21 cm observations and with an [O III]/[O II] (5007/3727) ratio of 18.3 ± 0.11, Pox 186 is a promising candidate Lyman continuum emitter. It may be a possible analog of …

2021 The Astrophysical Journal
eHST 12