Search Publications

An Analysis of ALMA Deep Fields and the Perceived Dearth of High-z Galaxies
DOI: 10.3847/1538-4357/aacd11 Bibcode: 2018ApJ...862...78C

Finkelstein, Steven L.; Casey, Caitlin M.; Zavala, Jorge A. +5 more

Deep, pencil-beam surveys from ALMA at 1.1-1.3 mm have uncovered an apparent absence of high-redshift dusty galaxies, with existing redshift distributions peaking around z ∼ 1.5-2.5. This has led to a perceived dearth of dusty systems at z ≳ 4 and the conclusion, according to some models, that the early universe was relatively dust-poor. In this p…

2018 The Astrophysical Journal
eHST 55
K2-141 b. A 5-M super-Earth transiting a K7 V star every 6.7 h
DOI: 10.1051/0004-6361/201732217 Bibcode: 2018A&A...612A..95B

Deeg, H.; Erikson, A.; Fridlund, M. +32 more

We report on the discovery of K2-141 b (EPIC 246393474 b), an ultra-short-period super-Earth on a 6.7 h orbit transiting an active K7 V star based on data from K2 campaign 12. We confirmed the planet's existence and measured its mass with a series of follow-up observations: seeing-limited MuSCAT imaging, NESSI high-resolution speckle observations,…

2018 Astronomy and Astrophysics
Gaia 55
Two Episodes of Magnetic Reconnections during a Confined Circular-ribbon Flare
DOI: 10.3847/1538-4357/aabe84 Bibcode: 2018ApJ...859..122L

Hou, Yijun; Li, Ting; Yang, Shuhong +2 more

We analyze a unique event with an M1.8 confined circular-ribbon flare on 2016 February 13, with successive formations of two circular ribbons at the same location. The flare had two distinct phases of UV and extreme ultraviolet emissions with an interval of about 270 s, of which the second peak was energetically more important. The first episode w…

2018 The Astrophysical Journal
IRIS 55
CME-driven Shock and Type II Solar Radio Burst Band Splitting
DOI: 10.3847/1538-4357/aae9e5 Bibcode: 2018ApJ...868...79C

Temmer, Manuela; Kontar, Eduard P.; Chrysaphi, Nicolina +1 more

Coronal mass ejections (CMEs) are believed to be effective in producing shocks in the solar corona and interplanetary space. One of the important signatures of shocks and shock acceleration are Type II solar radio bursts that drift with the shock speed and produce bands of fundamental and higher harmonic plasma radio emission. An intriguing aspect…

2018 The Astrophysical Journal
SOHO 55
IRIS and SDO Observations of Solar Jetlets Resulting from Network-edge Flux Cancelation
DOI: 10.3847/2041-8213/aaef37 Bibcode: 2018ApJ...868L..27P

Tiwari, Sanjiv K.; De Pontieu, Bart; Panesar, Navdeep K. +3 more

Recent observations show that the buildup and triggering of minifilament eruptions that drive coronal jets result from magnetic flux cancelation at the neutral line between merging majority- and minority-polarity magnetic flux patches. We investigate the magnetic setting of 10 on-disk small-scale UV/EUV jets (jetlets, smaller than coronal X-ray je…

2018 The Astrophysical Journal
IRIS 55
Spatially resolved cold molecular outflows in ULIRGs
DOI: 10.1051/0004-6361/201833089 Bibcode: 2018A&A...616A.171P

Rigopoulou, D.; Colina, L.; van der Werf, P. +11 more

We present new CO(2-1) observations of three low-z (d 350 Mpc) ultra-luminous infrared galaxy (ULIRG) systems (six nuclei) observed with the Atacama large millimeter/submillimeter array (ALMA) at high spatial resolution ( 500 pc). We detect massive cold molecular gas outflows in five out of six nuclei (Mout (0.3-5) × 108 M

2018 Astronomy and Astrophysics
eHST 55
Imaging Plasma Density Structures in the Soft X-Rays Generated by Solar Wind Charge Exchange with Neutrals
DOI: 10.1007/s11214-018-0504-7 Bibcode: 2018SSRv..214...79S

Holmström, M.; Read, A. M.; Wing, S. +32 more

Both heliophysics and planetary physics seek to understand the complex nature of the solar wind's interaction with solar system obstacles like Earth's magnetosphere, the ionospheres of Venus and Mars, and comets. Studies with this objective are frequently conducted with the help of single or multipoint in situ electromagnetic field and particle ob…

2018 Space Science Reviews
Cluster XMM-Newton 55
The spiral structure of the Milky Way
DOI: 10.1088/1674-4527/18/12/146 Bibcode: 2018RAA....18..146X

Xu, Ye; Hou, Li-Gang; Wu, Yuan-Wei

The morphology and kinematics of the spiral structure of the Milky Way are long-standing problems in astrophysics. In this review we firstly summarize various methods with different tracers used to solve this puzzle. The astrometry of Galactic sources is gradually alleviating this difficult situation caused mainly by large distance uncertainties, …

2018 Research in Astronomy and Astrophysics
Gaia 55
Global-Mode Analysis of Full-Disk Data from the Michelson Doppler Imager and the Helioseismic and Magnetic Imager
DOI: 10.1007/s11207-017-1201-5 Bibcode: 2018SoPh..293...29L

Schou, Jesper; Larson, Timothy P.

Building upon our previous work, in which we analyzed smoothed and subsampled velocity data from the Michelson Doppler Imager (MDI), we extend our analysis to unsmoothed, full-resolution MDI data. We also present results from the Helioseismic and Magnetic Imager (HMI), in both full resolution and processed to be a proxy for the low-resolution MDI …

2018 Solar Physics
SOHO 55
Statistical Analysis of Torus and Kink Instabilities in Solar Eruptions
DOI: 10.3847/1538-4357/aad6e4 Bibcode: 2018ApJ...864..138J

Xu, Yan; Liu, Chang; Jing, Ju +4 more

A recent laboratory experiment of ideal magnetohydrodynamic instabilities revealed four distinct eruption regimes readily distinguished by the torus instability (TI) and helical kink instability (KI) parameters. To establish its observational counterpart, we collected 38 solar flares (stronger than GOES-class M5 in general) that took place within …

2018 The Astrophysical Journal
SOHO 55