Search Publications

Discovery of 18 Stars with -3.10 < [Fe/H] < -1.45 in the Sagittarius Dwarf Galaxy
DOI: 10.3847/1538-4357/abb1ae Bibcode: 2020ApJ...901..164C

Frebel, Anna; Chiti, Anirudh; Hansen, Kylie Y.

Studies of the early chemical evolution of some larger dwarf galaxies (>107 M) are limited by the small number of stars known at low metallicities in these systems. Here we present metallicities and carbon abundances for eighteen stars with metallicities between -3.08 ≤ [Fe/H] ≤ -1.47 in the Sagittarius dwarf spheroidal g…

2020 The Astrophysical Journal
Gaia 16
The Streamer Blowout Origin of a Flux Rope and Energetic Particle Event Observed by Parker Solar Probe at 0.5 au
DOI: 10.3847/1538-4357/ab9942 Bibcode: 2020ApJ...897..134L

Luhmann, J. G.; Lario, D.; Arge, C. N. +18 more

The distribution of spacecraft in the inner heliosphere during 2019 March enabled comprehensive observations of an interplanetary coronal mass ejection (ICME) that encountered Parker Solar Probe (PSP) at 0.547 au from the Sun. This ICME originated as a slow (∼311 km s-1) streamer blowout (SBO) on the Sun as measured by the white-light c…

2020 The Astrophysical Journal
SOHO 16
Detection of the Red Supergiant Wind from the Progenitor of Cassiopeia A
DOI: 10.3847/1538-4357/ab76bf Bibcode: 2020ApJ...891..116W

Chevalier, Roger A.; Raymond, John C.; Milisavljevic, Dan +4 more

Cassiopeia A (Cas A) is one of the best studied young Galactic supernova remnants. While it provides a rare opportunity to study in detail the remnant of a supernova (SN) type IIb, questions remain regarding the nature of its progenitor, its mass-loss history, and its pre-SN evolution. Here we present an optical investigation of the circumstellar …

2020 The Astrophysical Journal
eHST 16
The Warm Gas in the MW: A Kinematical Model
DOI: 10.3847/1538-4357/ab774e Bibcode: 2020ApJ...894..142Q

Bregman, Joel N.; Qu, Zhijie; Lindley, Ryan +2 more

We develop a kinematical model for the Milky Way Si IV-bearing gas to determine its density distribution and kinematics. This model is constrained by a column density line-shape sample extracted from the Hubble Space Telescope/Cosmic Origins Spectrograph archival data, which contains 186 active galactic nucleus sight lines. We find that the Si IV …

2020 The Astrophysical Journal
IUE eHST 16
ZFIRE: Measuring Electron Density with [O II] as a Function of Environment at z = 1.62
DOI: 10.3847/1538-4357/ab76cf Bibcode: 2020ApJ...892...77H

Papovich, Casey; Kewley, Lisa J.; Harshan, Anishya +8 more

The global star formation rates (SFR) of galaxies at fixed stellar masses increase with redshift and are known to vary with environment up to z ∼ 2. We explore here whether the changes in the SFRs also apply to the electron densities of the interstellar medium by measuring the [O II] (λ 3726, λ 3729) ratio for cluster and field galaxies at z ∼ 2. …

2020 The Astrophysical Journal
eHST 16
On the Coronal Temperature in Solar Microflares
DOI: 10.3847/1538-4357/abb36e Bibcode: 2020ApJ...902...31T

Testa, Paola; Reale, Fabio

We present a study of solar imaging and spectral observations of a microflare, focusing on the temperature diagnostics provided by the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamics Observatory, and the Extreme-Ultraviolet Imaging Spectrometer (EIS) on board Hinode. Our data analysis, in particular from the emission in the 131 and …

2020 The Astrophysical Journal
Hinode 16
On the Relation between the Hard X-Ray Photon Index and Accretion Rate for Super-Eddington Accreting Quasars
DOI: 10.3847/1538-4357/ab9019 Bibcode: 2020ApJ...895..114H

Luo, Bin; Huang, Jian; Du, Pu +3 more

We investigate whether the correlation between the hard X-ray photon index ( ${\rm{\Gamma }}$ ) and accretion rate for super-Eddington accreting quasars is different from that for sub-Eddington accreting quasars. We construct a sample of 113 bright quasars from the Sloan Digital Sky Survey Data Release 14 quasar catalog, with 38 quasars as the sup…

2020 The Astrophysical Journal
XMM-Newton 16
Steady Wind-blown Cavities within Infalling Rotating Envelopes: Application to the Broad Velocity Component in Young Protostars
DOI: 10.3847/1538-4357/aba830 Bibcode: 2020ApJ...900...15L

Johnstone, Doug; Cabrit, Sylvie; Kristensen, Lars E. +1 more

Wind-driven outflows are observed around a broad range of accreting objects throughout the universe, ranging from forming low-mass stars to supermassive black holes. We study the interaction between a central isotropic wind and an infalling, rotating envelope, which determines the steady-state cavity shape formed at their interface under the assum…

2020 The Astrophysical Journal
Herschel 15
A Small-scale Filament Eruption Inducing a Moreton Wave, an EUV Wave, and a Coronal Mass Ejection
DOI: 10.3847/1538-4357/ab8565 Bibcode: 2020ApJ...894...30W

Xue, Zhike; Yan, Xiaoli; Wang, Jincheng +3 more

With the launch of the Solar Dynamic Observatory, many extreme ultraviolet (EUV) waves have been observed during solar eruptions. However, joint observations of Moreton and EUV waves are still relatively rare. We present an event in active region NOAA 12740 wherein a small-scale filament eruption simultaneously results in a Moreton wave, an EUV wa…

2020 The Astrophysical Journal
SOHO 15
Statistical Analysis of the Relation between Coronal Mass Ejections and Solar Energetic Particles
DOI: 10.3847/1538-4357/aba621 Bibcode: 2020ApJ...900...75K

Yashiro, Seiji; Nitta, Nariaki V.; Ichimoto, Kiyoshi +4 more

To improve the forecasting capability of impactful solar energetic particle (SEP) events, the relation between coronal mass ejections (CMEs) and SEP events needs to be better understood. Here we present a statistical study of SEP occurrences and timescales with respect to the CME source locations and speeds, considering all 257 fast (vCME

2020 The Astrophysical Journal
SOHO 15