Search Publications

Energetic Electron Acceleration in Unconfined Reconnection Jets
DOI: 10.3847/2041-8213/ab3041 Bibcode: 2019ApJ...881L...8C

Xu, Y.; Zhang, Y.; Chen, G. +5 more

Magnetic reconnection in astronomical objects such as solar corona and the Earth’s magnetotail theoretically produces a fast jet toward the object (known as a confined jet as it connects to the object through magnetic field lines) and a fast jet departing the object (known as an unconfined jet as it propagates freely in space). So far, energetic e…

2019 The Astrophysical Journal
Cluster 24
Impacts of EUV Wavefronts on Coronal Structures in Homologous Coronal Mass Ejections
DOI: 10.3847/1538-4357/aaf04e Bibcode: 2019ApJ...870...15L

Wang, Yuming; Shen, Chenglong; Liu, Rui +1 more

Large-scale propagating fronts are frequently observed during solar eruptions, yet whether or not they are waves is an open question, partly because the propagation is modulated by coronal structures, whose magnetic fields we still cannot measure. However, when a front impacts coronal structures, an opportunity arises for us to look into the magne…

2019 The Astrophysical Journal
SOHO 24
High-resolution Near-infrared Spectroscopy of HD 100546. IV. Orbiting Companion Disappears on Schedule
DOI: 10.3847/1538-4357/ab380b Bibcode: 2019ApJ...883...37B

Najita, Joan R.; Brittain, Sean D.; Carr, John S.

HD 100546 is a Herbig Ae/Be star surrounded by a disk with a large central region that is cleared of gas and dust (i.e., an inner hole). High-resolution near-infrared spectroscopy reveals a rich emission spectrum of fundamental rovibrational CO emission lines whose time variable properties point to the presence of an orbiting companion within the …

2019 The Astrophysical Journal
Gaia 24
Stronger Constraints on the Evolution of the M BH-{\sigma }_{* } Relation up to z ∼ 0.6
DOI: 10.3847/1538-4357/ab21d5 Bibcode: 2019ApJ...878..101S

Canalizo, Gabriela; Sexton, Remington O.; Treister, Ezequiel +4 more

We revisit the possibility of redshift evolution in the M BH* relation with a sample of 22 Seyfert 1 galaxies with black holes (BHs) in the mass range {10}6.3{--}{10}8.3 {M} and redshift range 0.03 < z < 0.57 with spectra obtained from spatially resolved Keck/Low-resolution Imaging …

2019 The Astrophysical Journal
eHST 24
Unbiased Cosmological Parameter Estimation from Emission-line Surveys with Interlopers
DOI: 10.3847/1538-4357/ab12d5 Bibcode: 2019ApJ...876...32G

Schneider, Donald P.; Gebhardt, Karl; Ciardullo, Robin +11 more

The galaxy catalogs generated from low-resolution emission-line surveys often contain both foreground and background interlopers due to line misidentification, which can bias the cosmological parameter estimation. In this paper, we present a method for correcting the interloper bias by using the joint analysis of auto- and cross-power spectra of t…

2019 The Astrophysical Journal
eHST 24
Different Signatures of Chromospheric Evaporation in Two Solar Flares Observed with IRIS
DOI: 10.3847/1538-4357/ab245a Bibcode: 2019ApJ...879...30L

Gan, W. Q.; Ding, M. D.; Li, H. +2 more

We present different signatures of chromospheric evaporation in two solar flares observed by the Interface Region Imaging Spectrograph (IRIS). In the B1.6 flare on 2016 December 6 (SOL2016-12-06T10:40), the transition region Si IV line and the chromospheric C II and Mg II lines show blueshifts with low velocities up to 20 km s-1 at the …

2019 The Astrophysical Journal
IRIS 24
CWISEP J193518.59-154620.3: An Extremely Cold Brown Dwarf in the Solar Neighborhood Discovered with CatWISE
DOI: 10.3847/1538-4357/ab2bf0 Bibcode: 2019ApJ...881...17M

Teplitz, Harry I.; Schlegel, David J.; Mobasher, Bahram +17 more

We present the discovery of an extremely cold, nearby brown dwarf in the solar neighborhood, found in the CatWISE catalog. Photometric follow-up with Spitzer reveals that the object, CWISEP J193518.59-154620.3, has ch1-ch2 = 3.24 ± 0.31 mag, making it one of the reddest brown dwarfs known. Using the Spitzer photometry and the polynomial relations …

2019 The Astrophysical Journal
Gaia 24
A Confined Partial Eruption of Double-decker Filaments
DOI: 10.3847/1538-4357/ab0f3f Bibcode: 2019ApJ...875...71Z

Yang, Shuhong; Chen, Yao; Zheng, Ruisheng +6 more

Filament eruptions, one of the most energetic explosions on the Sun, release large quantities of magnetized plasma into the interplanetary space. Hence, the understanding of the initiation and evolution of filament eruptions can provide broader implications for space weather and geospace climate. Here, we present a confined partial eruption of dou…

2019 The Astrophysical Journal
Hinode 24
The Most Massive Galaxies with Large Depleted Cores: Structural Parameter Relations and Black Hole Masses
DOI: 10.3847/1538-4357/ab4d4f Bibcode: 2019ApJ...886...80D

Dullo, Bililign T.

Luminous spheroids (M V ≲ -21.50 ± 0.75 mag) contain partially depleted cores with sizes (R b) typically 0.02-0.5 kpc. However, galaxies with R b > 0.5 kpc are rare and poorly understood. Here, we perform detailed decompositions of the composite surface brightness profiles, extracted from archival Hubble Space…

2019 The Astrophysical Journal
eHST 24
Spatially Resolved Metal Loss from M31
DOI: 10.3847/1538-4357/ab1b3f Bibcode: 2019ApJ...877..120T

Williams, Benjamin F.; Dalcanton, Julianne J.; Werk, Jessica K. +1 more

As galaxies evolve, they must enrich and exchange gas with the surrounding medium, but the timing of these processes and how much gas is involved remain poorly understood. In this work, we leverage metals as tracers of past gas flows to constrain the history of metal ejection and redistribution in M31. This roughly L* galaxy is a unique case where…

2019 The Astrophysical Journal
eHST 24