Search Publications

Observations of Turbulent Magnetic Reconnection within a Solar Current Sheet
DOI: 10.3847/1538-4357/aadd16 Bibcode: 2018ApJ...866...64C

Cheng, X.; Ding, M. D.; Zhang, J. +4 more

Magnetic reconnection is a fundamental physical process in various astrophysical, space, and laboratory environments. Many pieces of evidence for magnetic reconnection have been uncovered. However, its specific processes that could be fragmented and turbulent have been short of direct observational evidence. Here, we present observations of a supe…

2018 The Astrophysical Journal
Hinode SOHO 127
Kiloparsec-scale gaseous clumps and star formation at z = 5-7
DOI: 10.1093/mnras/sty1088 Bibcode: 2018MNRAS.478.1170C

Maiolino, R.; Castellano, M.; Pentericci, L. +13 more

We investigate the morphology of the [C II] emission in a sample of `normal' star-forming galaxies at 5 < z < 7.2 in relation to their UV (rest-frame) counterpart. We use new Atacama Large Millimetre/submillimetre Array (ALMA) observations of galaxies at z ∼ 6-7, as well as a careful re-analysis of archival ALMA data. In total 29 galaxies we…

2018 Monthly Notices of the Royal Astronomical Society
Gaia eHST 126
OSSOS. VII. 800+ Trans-Neptunian Objects—The Complete Data Release
DOI: 10.3847/1538-4365/aab77a Bibcode: 2018ApJS..236...18B

Murray-Clay, Ruth; Granvik, Mikael; Wang, Shiang-Yu +33 more

The Outer Solar System Origins Survey (OSSOS), a wide-field imaging program in 2013-2017 with the Canada-France-Hawaii Telescope, surveyed 155 deg2 of sky to depths of m r = 24.1-25.2. We present 838 outer solar system discoveries that are entirely free of ephemeris bias. This increases the inventory of trans-Neptunian obje…

2018 The Astrophysical Journal Supplement Series
Gaia 126
Gaia Data Release 2. Processing the spectroscopic data
DOI: 10.1051/0004-6361/201832836 Bibcode: 2018A&A...616A...6S

Smith, M.; Gosset, E.; Allende Prieto, C. +50 more

Context. The Gaia Data Release 2 (DR2) contains the first release of radial velocities complementing the kinematic data of a sample of about 7 million relatively bright, late-type stars.
Aims: This paper provides a detailed description of the Gaia spectroscopic data processing pipeline, and of the approach adopted to derive the radial velocit…

2018 Astronomy and Astrophysics
Gaia 125
3D mapping of young stars in the solar neighbourhood with Gaia DR2
DOI: 10.1051/0004-6361/201834150 Bibcode: 2018A&A...620A.172Z

Brown, A. G. A.; Jardine, K.; de Zeeuw, P. T. +2 more

We study the three dimensional arrangement of young stars in the solar neighbourhood using the second release of the Gaia mission (Gaia DR2) and we provide a new, original view of the spatial configuration of the star-forming regions within 500 pc of the Sun. By smoothing the star distribution through a Gaussian filter, we construct three dimensio…

2018 Astronomy and Astrophysics
Gaia 125
Short GRBs: Opening Angles, Local Neutron Star Merger Rate, and Off-axis Events for GRB/GW Association
DOI: 10.3847/1538-4357/aab76d Bibcode: 2018ApJ...857..128J

Li, Xiang; Yuan, Qiang; Jin, Zhi-Ping +7 more

The jet breaks in the afterglow light curves of short gamma-ray bursts (SGRBs), rarely detected so far, are crucial for estimating the half-opening angles of the ejecta (θ j) and hence the neutron star merger rate. In this work, we report the detection of jet decline behaviors in GRB 150424A and GRB 160821B, and find θ j ∼ 0.…

2018 The Astrophysical Journal
eHST 124
The Gaia 20 pc white dwarf sample
DOI: 10.1093/mnras/sty2057 Bibcode: 2018MNRAS.480.3942H

Gänsicke, B. T.; Tremblay, P. -E.; Hollands, M. A. +2 more

Using Gaia DR2 data, we present an up-to-date sample of white dwarfs within 20 pc of the Sun. In total we identified 139 systems in Gaia DR2, nine of which are new detections, with the closest of these located at a distance of 13.05 pc. We estimated atmospheric parameters for all stellar remnants based on the Gaia parallaxes and photometry. The hi…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 123
The MUSCLES Treasury Survey. V. FUV Flares on Active and Inactive M Dwarfs
DOI: 10.3847/1538-4357/aae2bd Bibcode: 2018ApJ...867...71L

Loyd, R. O. Parke; Redfield, Seth; Brown, Alexander +10 more

M dwarf stars are known for their vigorous flaring. This flaring could impact the climate of orbiting planets, making it important to characterize M dwarf flares at the short wavelengths that drive atmospheric chemistry and escape. We conducted a far-ultraviolet flare survey of six M dwarfs from the recent MUSCLES (Measurements of the Ultraviolet …

2018 The Astrophysical Journal
XMM-Newton eHST 123
Measuring the Physical Conditions in High-redshift Star-forming Galaxies: Insights from KBSS-MOSFIRE
DOI: 10.3847/1538-4357/aae1a5 Bibcode: 2018ApJ...868..117S

Pettini, Max; Steidel, Charles C.; Rudie, Gwen C. +2 more

We use photoionization models that are designed to reconcile the joint rest-UV-optical spectra of high-z star-forming galaxies to self-consistently infer the gas chemistry and nebular ionization and excitation conditions for ∼150 galaxies from the Keck Baryonic Structure Survey (KBSS), using only observations of their rest-optical nebular spectra.…

2018 The Astrophysical Journal
eHST 123
BANYAN. XIII. A First Look at Nearby Young Associations with Gaia Data Release 2
DOI: 10.3847/1538-4357/aaca2e Bibcode: 2018ApJ...862..138G

Faherty, Jacqueline K.; Gagné, Jonathan

In this paper, we examine the nearest 100 pc entries in Data Release 2 of Gaia to identify previously unrecognized candidate members in young associations. We analyze 695 952 stars with the BANYAN Σ Bayesian classification software and discover 898 new high-likelihood candidate members that span a wide range of properties, from spectral types B9 t…

2018 The Astrophysical Journal
Gaia 122