Search Publications

Does Nearby Open Flux Affect the Eruptivity of Solar Active Regions?
DOI: 10.3847/1538-4357/aac77a Bibcode: 2018ApJ...861..131D

DeRosa, Marc L.; Barnes, Graham

The most energetic solar flares are typically associated with the ejection of a cloud of coronal material into the heliosphere in the form of a coronal mass ejection (CME). However, large flares exist that are not accompanied by a CME. The existence of these noneruptive flares raises the question of whether such flares suffer from a lack of access…

2018 The Astrophysical Journal
SOHO 13
The Envelope Kinematics and a Possible Disk around the Class 0 Protostar within BHR7
DOI: 10.3847/1538-4357/aaafc7 Bibcode: 2018ApJ...856..164T

Bourke, Tyler L.; Dunham, Michael M.; Tobin, John J. +2 more

We present a characterization of the protostar embedded within the BHR7 dark cloud, based on both photometric measurements from the near-infrared to millimeter and interferometric continuum and molecular line observations at millimeter wavelengths. We find that this protostar is a Class 0 system, the youngest class of protostars, measuring its bol…

2018 The Astrophysical Journal
Herschel 13
Constraining the parameter space of comet simulation experiments
DOI: 10.1016/j.icarus.2018.03.025 Bibcode: 2018Icar..311..105K

Hagermann, Axel; Kaufmann, Erika

Our interpretation of the data returned by Rosetta and other cometary missions is based on the predictions of theoretical models and the results of laboratory experiments. For example, Kossacki et al. (2015) showed that 67P's surface hardness reported by Spohn et al. (2015) can be explained by sintering. The present work supports Rosetta's observa…

2018 Icarus
Rosetta 13
Bright Network, UVA, and the Physical Modeling of Solar Spectral and Total Irradiance in Recent Solar Cycles
DOI: 10.3847/1538-4357/aac388 Bibcode: 2018ApJ...861..120F

Fontenla, J. M.; Landi, E.

In this paper we study the total solar irradiance (TSI) and the spectral solar irradiance (SSI) by applying the solar disk image decomposition algorithm (SDIDA) and solar irradiance synthesis algorithm (SISA) methods. These methods were applied to space-based observations in previous works, but in this work, they are applied to ground-based observ…

2018 The Astrophysical Journal
SOHO 13
Quantifying Turbulent Dynamics Found within the Plasma Sheets of Multiple Solar Flares
DOI: 10.3847/1538-4357/aadee4 Bibcode: 2018ApJ...866...29F

McKenzie, David E.; Freed, Michael S.

It is vital to our understanding of solar flares that we discern how turbulent motion can affect the magnetic reconnection process. The objective of this study is to quantify the velocity and vorticity structures inherent in the observed motions found in a plasma sheet above arcades during a solar flare. The most noticeable features in these plasm…

2018 The Astrophysical Journal
Hinode 13
Reconstruction of asteroid spin states from Gaia DR2 photometry
DOI: 10.1051/0004-6361/201834007 Bibcode: 2018A&A...620A..91D

Hanuš, J.; Ďurech, J.

Context. In addition to stellar data, Gaia Data Release 2 (DR2) also contains accurate astrometry and photometry of about 14 000 asteroids covering 22 months of observations.
Aims: We used Gaia asteroid photometry to reconstruct rotation periods, spin axis directions, and the coarse shapes of a subset of asteroids with enough observations. On…

2018 Astronomy and Astrophysics
Gaia 13
Accurate radial velocity and metallicity of the Large Magellanic Cloud old globular clusters NGC 1928 and NGC 1939
DOI: 10.1093/mnras/sty2324 Bibcode: 2018MNRAS.481...49P

Cole, A. A.; Hwang, N.; Angelo, M. S. +2 more

We present results obtained from spectroscopic observations of red giants located in the fields of the Large Magellanic Cloud (LMC) globular clusters (GCs) NGC 1928 and NGC 1939. We used the GMOS and AAOmega+2dF spectrographs to obtain spectra centred on the Ca II triplet, from which we derived individual radial velocities (RVs) and metallicities.…

2018 Monthly Notices of the Royal Astronomical Society
Gaia eHST 13
A Seasonally Recurrent Annular Cyclone in Mars Northern Latitudes and Observations of a Companion Vortex
DOI: 10.1029/2018JE005740 Bibcode: 2018JGRE..123.3020S

Gondet, B.; Forget, F.; Hueso, R. +12 more

We study a seasonally recurrent cyclone and related cloud phenomena observed on Mars at Ls 120°, latitude 60°N, and longitude 90°W from images obtained with cameras in different spacecraft between 1995 and 2018. A remarkable double cyclone formed in 2012 and we present a detailed study of its dynamics using images from Mars Express and …

2018 Journal of Geophysical Research (Planets)
MEx 13
The oxygen isotopic composition (18O/16O) in the dust of comet 67P/Churyumov-Gerasimenko measured by COSIMA on-board Rosetta
DOI: 10.1093/mnras/sty560 Bibcode: 2018MNRAS.477.3836P

Hilchenbach, M.; Engrand, C.; Kissel, J. +5 more

The oxygen isotopic ratio 18O/16O has been measured in cometary gas for a wide variety of comets, but the only measurements in cometary dust were performed by the Stardust cometary sample return mission. Most such measurements find a value of the ratio that is consistent with Vienna Standard Mean Ocean Water (VSMOW) within er…

2018 Monthly Notices of the Royal Astronomical Society
Rosetta 13
The Advanced Spectral Library (ASTRAL): Reference Spectra for Evolved M Stars
DOI: 10.3847/1538-4357/aaf164 Bibcode: 2018ApJ...869..157C

Ayres, Thomas R.; Carpenter, Kenneth G.; Nielsen, Krister E. +3 more

The HST Treasury Program Advanced Spectral Library Project: Cool Stars was designed to collect representative, high-quality UV spectra of eight evolved F-M type cool stars. The Space Telescope Imaging Spectrograph (STIS) echelle spectra of these objects enable investigations of a broad range of topics, including stellar and interstellar astrophysi…

2018 The Astrophysical Journal
eHST 13