Search Publications

Evidence for Centrifugal Breakout around the Young M Dwarf TIC 234284556
DOI: 10.3847/1538-4357/ac38a5 Bibcode: 2022ApJ...925...75P

Montet, Benjamin T.; Hartman, Joel D.; Feinstein, Adina D. +5 more

Magnetospheric clouds have been proposed as explanations for depth-varying dips in the phased light curves of young, magnetically active stars such as σ Ori E and RIK-210. However, the stellar theory that first predicted magnetospheric clouds also anticipated an associated mass-balancing mechanism known as centrifugal breakout for which there has …

2022 The Astrophysical Journal
Gaia 9
The Internal Proper Motion Kinematics of NGC 346: Past Formation and Future Evolution
DOI: 10.3847/1538-4357/ac8005 Bibcode: 2022ApJ...936..135S

Anderson, J.; Lennon, D. J.; Sabbi, E. +6 more

We investigate the internal kinematics of the young star-forming region NGC 346 in the Small Magellanic Cloud (SMC). We used two epochs of deep F555W and F814W Hubble Space Telescope Advanced Camera for Surveys observations with an 11 yr baseline to determine proper motions and study the kinematics of different populations, as identified by their …

2022 The Astrophysical Journal
Gaia eHST 9
New Constraints on Cosmic Particle Populations at the Galactic Center Using X-Ray Observations of the Molecular Cloud Sagittarius B2
DOI: 10.3847/1538-4357/ac7717 Bibcode: 2022ApJ...934...19R

Zhang, Shuo; Clavel, Maïca; Perez, Kerstin +2 more

The Sagittarius B2 (Sgr B2) molecular cloud complex is an X-ray reflection nebula whose nonthermal X-ray emissions have continued to decrease since 2001 as it reprocesses one or more past energetic outbursts from the supermassive black hole Sagittarius A* at the Galactic Center. The X-ray reflection model explains the observed time variability of …

2022 The Astrophysical Journal
Herschel XMM-Newton 9
Acceleration and Expansion of a Coronal Mass Ejection in the High Corona: Role of Magnetic Reconnection
DOI: 10.3847/1538-4357/ac75d4 Bibcode: 2022ApJ...933..169Z

Temmer, Manuela; Lugaz, Noé; Zhuang, Bin +2 more

The important role played by magnetic reconnection in the early acceleration of coronal mass ejections (CMEs) has been widely discussed. However, as CMEs may have expansion speeds comparable to their propagation speeds in the corona, it is not clear whether and how reconnection contributes to the true acceleration and expansion separately. To addr…

2022 The Astrophysical Journal
SOHO 9
A Long-period Pre-ELM System Discovered from the LAMOST Medium-resolution Survey
DOI: 10.3847/1538-4357/ac75b6 Bibcode: 2022ApJ...933..193Z

Liu, Jifeng; Bai, Yu; Gu, Wei-Min +16 more

We present LAMOST J041920.07+072545.4 (hereafter J0419), a close binary consisting of a bloated, extremely low mass pre-white dwarf (pre-ELM WD) and a compact object with an orbital period of 0.607189 days. The large-amplitude ellipsoidal variations and the evident Balmer and He I emission lines suggest a filled Roche lobe and ongoing mass transfe…

2022 The Astrophysical Journal
Gaia 9
Evolution of Plasma Composition in an Eruptive Flux Rope
DOI: 10.3847/1538-4357/ac32d2 Bibcode: 2022ApJ...924...17B

Long, D. M.; van Driel-Gesztelyi, L.; Démoulin, P. +8 more

Magnetic flux ropes are bundles of twisted magnetic field enveloping a central axis. They harbor free magnetic energy and can be progenitors of coronal mass ejections (CMEs). However, identifying flux ropes on the Sun can be challenging. One of the key coronal observables that has been shown to indicate the presence of a flux rope is a peculiar br…

2022 The Astrophysical Journal
Hinode SOHO 9
Deep Learning Based Solar Flare Forecasting Model. II. Influence of Image Resolution
DOI: 10.3847/1538-4357/ac99dc Bibcode: 2022ApJ...941...20L

Liu, Sixuan; Xu, Long; Zhao, Zhongrui +3 more

Due to the accumulation of solar observational data and the development of data-driven algorithms, deep learning methods are widely applied to build a solar flare forecasting model. Most of the works focus on how to design or select proper deep networks for the forecasting task. Nevertheless, the influence of image resolution on the learning based…

2022 The Astrophysical Journal
Hinode SOHO 9
3D-DASH: The Widest Near-infrared Hubble Space Telescope Survey
DOI: 10.3847/1538-4357/ac71af Bibcode: 2022ApJ...933..129M

van Dokkum, Pieter G.; Franx, Marijn; Muzzin, Adam +15 more

The 3D-Drift And SHift (3D-DASH) program is a Hubble Space Telescope (HST) WFC3 F160W imaging and G141 grism survey of the equatorial COSMOS field. 3D-DASH extends the legacy of HST near-infrared imaging and spectroscopy to degree-scale swaths of the sky, enabling the identification and study of distant galaxies (z > 2) that are rare or in shor…

2022 The Astrophysical Journal
eHST 9
Kiloparsec-scale Imaging of the CO(1-0)-traced Cold Molecular Gas Reservoir in a z 3.4 Submillimeter Galaxy
DOI: 10.3847/1538-4357/ac6105 Bibcode: 2022ApJ...930...35F

van der Werf, Paul; Walter, Fabian; Narayanan, Desika +9 more

We present a high-resolution study of the cold molecular gas as traced by CO(1-0) in the unlensed z ~ 3.4 submillimeter galaxy SMM J13120+4242, using multiconfiguration observations with the Karl G. Jansky Very Large Array (JVLA). The gas reservoir, imaged on 0.″39 (~3 kpc) scales, is resolved into two components separated by ~11 kpc with a total …

2022 The Astrophysical Journal
eHST 9
Li Distribution, Kinematics, and Detailed Abundance Analysis among Very Metal-poor Stars in the Galactic Halo from the HESP-GOMPA Survey
DOI: 10.3847/1538-4357/ac8b0f Bibcode: 2022ApJ...937...52B

Beers, Timothy C.; Sivarani, Thirupathi; Pandey, Jeewan C. +3 more

We present a study on the detailed elemental abundances of newly identified, bright, very metal-poor stars with the detection of lithium, initially observed as part of the SDSS/MARVELS pre-survey. These stars were selected for high-resolution spectroscopic follow-up as part of the HESP-GOMPA survey. In this work, we discuss the Li abundances detec…

2022 The Astrophysical Journal
Gaia 9