Search Publications

The Formation Process of the First Halo Coronal Mass Ejection in Solar Cycle 25: Magnetic Cancellation, Bidirectional Jet, and Hot Channel
DOI: 10.3847/1538-4357/ac116d Bibcode: 2021ApJ...919...34Y

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

To better understand the trigger mechanism of a coronal mass ejection (CME), we present the evolution of a CME source region (active region NOAA 12790) and the formation of a hot channel before the occurrence of the first halo CME in solar cycle 25. Through analyzing the evolution of Solar Dynamics Observatory/Helioseismic and Magnetic Imager line…

2021 The Astrophysical Journal
SOHO 13
Longitudinally Resolved Spectral Retrieval (ReSpect) of WASP-43b
DOI: 10.3847/1538-4357/abfe14 Bibcode: 2021ApJ...915...45C

Gonzales, Eileen C.; Cubillos, Patricio E.; Cowan, Nicolas B. +6 more

Thermal phase variations of short-period planets indicate that they are not spherical cows: day-to-night temperature contrasts range from hundreds to thousands of degrees, rivaling their vertical temperature contrasts. Nonetheless, the emergent spectra of short-period planets have typically been fit using one-dimensional (1D) spectral retrieval co…

2021 The Astrophysical Journal
eHST 13
Synthetic Absorption Lines from Simulations of Multiphase Gas in Galactic Winds
DOI: 10.3847/1538-4357/ac04ac Bibcode: 2021ApJ...919..112D

Ostriker, Eve C.; de la Cruz, Lita M.; Schneider, Evan E.

Supernova-driven galactic winds are multiphase streams of gas that are often observed flowing at a range of velocities out of star-forming regions in galaxies. In this study, we use high-resolution 3D simulations of multiphase galactic winds modeled with the hydrodynamics code Cholla to investigate the connection between numerical studies and obse…

2021 The Astrophysical Journal
eHST 13
Late-time Hubble Space Telescope Observations of a Hydrogen-poor Superluminous Supernova Reveal the Power-law Decline of a Magnetar Central Engine
DOI: 10.3847/1538-4357/ac1b27 Bibcode: 2021ApJ...921...64B

Berger, Edo; Chornock, Ryan; Nicholl, Matt +3 more

The light-curve diversity of hydrogen-poor superluminous supernovae (SLSNe) has kept open the possibility that multiple power sources account for the population. Specifically, pair-instability explosions (PISNe), which produce large masses of 56Ni, have been argued as the origin of some slowly-evolving SLSNe. Here we present detailed ob…

2021 The Astrophysical Journal
eHST 13
Solar Modulation of Galactic Cosmic-Ray Protons Based on a Modified Force-field Approach
DOI: 10.3847/1538-4357/ac1fe8 Bibcode: 2021ApJ...921..109S

Qin, Gang; Shen, Zhenning; Yang, Hao +4 more

In this work, a modified force-field approach is established to investigate the long-term solar modulation of galactic cosmic-ray (GCR) protons. In this approach, the solar modulation potential φ is assumed to be energy dependent. As φ also depends on the local interstellar spectrum (LIS), a new proton LIS model is first presented based on data fr…

2021 The Astrophysical Journal
SOHO 13
A LAMOST BHB Catalog and Kinematics Therein. I. Catalog and Halo Properties
DOI: 10.3847/1538-4357/abe4d0 Bibcode: 2021ApJ...912...32V

Shen, Juntai; Smith, Martin C.; Li, Zhao-Yu +1 more

In this paper, we collect a sample of stars observed both in LAMOST and Gaia, which have colors implying a temperature hotter than 7000 K. We train a machine-learning algorithm on LAMOST spectroscopic data which has been tagged with stellar classifications and metallicities, and use this machine to construct a catalog of blue horizontal branch sta…

2021 The Astrophysical Journal
Gaia 13
The Cepheid Distance to the Narrow-line Seyfert 1 Galaxy NGC 4051
DOI: 10.3847/1538-4357/abf24a Bibcode: 2021ApJ...913....3Y

Ferrarese, L.; Vestergaard, M.; Peterson, B. M. +15 more

We derive a distance of D = 16.6 ± 0.3 Mpc (µ = 31.10 ± 0.04 mag) to the archetypal narrow-line Seyfert 1 galaxy NGC 4051 based on Cepheid period-luminosity relations and new Hubble Space Telescope multiband imaging. We identify 419 Cepheid candidates and estimate the distance at both optical and near-infrared wavelengths using subsamples of…

2021 The Astrophysical Journal
eHST 13
The Isaac Newton Telescope Monitoring Survey of Local Group Dwarf Galaxies. II. The Star-formation History of Andromeda I Derived from Long-period Variables
DOI: 10.3847/1538-4357/ac2d96 Bibcode: 2021ApJ...923..164S

Javadi, Atefeh; Saremi, Elham; van Loon, Jacco Th. +4 more

An optical monitoring survey in the nearby dwarf galaxies was carried out with the 2.5 m Isaac Newton Telescope. 55 dwarf galaxies and four isolated globular clusters in the Local Group were observed with the Wide Field Camera. The main aims of this survey are to identify the most evolved asymptotic giant branch stars and red supergiants at the en…

2021 The Astrophysical Journal
Gaia 13
Spatially Resolved BPT Mapping of Nearby Seyfert 2 Galaxies
DOI: 10.3847/1538-4357/abcfc1 Bibcode: 2021ApJ...908..155M

Elvis, Martin; Storchi-Bergmann, Thaisa; Fabbiano, G. +5 more

We present spatially resolved Baldwin-Phillips-Terlevich (BPT) mapping of the extended narrow-line regions (ENLRs) of seven nearby Seyfert 2 galaxies, using Hubble Space Telescope narrowband filter imaging. We construct the BPT diagrams using ≤0"1 resolution emission line images of [O III] λ5007, Hα, [S II] λλ6717, 6731, and Hβ. By mapping these d…

2021 The Astrophysical Journal
eHST 13
Predicting the Spectrum of UGC 2885, Rubin's Galaxy with Machine Learning
DOI: 10.3847/1538-4357/abffcc Bibcode: 2021ApJ...914..142H

Holwerda, Benne W.; Bailin, Jeremy; Böker, Torsten +10 more

Wu & Peek predict SDSS-quality spectra based on Pan-STARRS broadband grizy images using machine learning (ML). In this article, we test their prediction for a unique object, UGC 2885 ("Rubin's galaxy"), the largest and most massive, isolated disk galaxy in the local universe (D < 100 Mpc). After obtaining the ML predicted spectrum, we compa…

2021 The Astrophysical Journal
eHST 13