Search Publications

Inferring Binary and Trinary Stellar Populations in Photometric and Astrometric Surveys
DOI: 10.3847/1538-4357/aab7ee Bibcode: 2018ApJ...857..114W

Leistedt, Boris; Hogg, David W.; Widmark, Axel

Multiple stellar systems are ubiquitous in the Milky Way but are often unresolved and seen as single objects in spectroscopic, photometric, and astrometric surveys. However, modeling them is essential for developing a full understanding of large surveys such as Gaia and connecting them to stellar and Galactic models. In this paper, we address this…

2018 The Astrophysical Journal
Gaia 13
The Detached Auroras Induced by the Solar Wind Pressure Enhancement in Both Hemispheres From Imaging and In Situ Particle Observations
DOI: 10.1002/2017JA024562 Bibcode: 2018JGRA..123.3170Z

Zhou, Su; Luan, Xiaoli; Søraas, Finn +2 more

This paper presents simultaneous detached proton auroras that appeared in both hemispheres at 11:06 UT, 08 March 2012, just 2 min after a sudden solar wind pressure enhancement ( 11:04 UT) hit the Earth. They were observed under northward interplanetary magnetic field Bz condition and during the recovery phase of a moderate geomagnetic storm. In t…

2018 Journal of Geophysical Research (Space Physics)
Cluster 13
The fast transient sky with Gaia
DOI: 10.1093/mnras/stx2625 Bibcode: 2018MNRAS.473.3854W

Jonker, Peter G.; van Leeuwen, Floor; Hodgkin, Simon T. +8 more

The ESA Gaia satellite scans the whole sky with a temporal sampling ranging from seconds and hours to months. Each time a source passes within the Gaia field of view, it moves over 10 charge coupled devices (CCDs) in 45 s and a light curve with 4.5 s sampling (the crossing time per CCD) is registered. Given that the 4.5 s sampling represents a vir…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 13
Evolution of the Auroral Signatures of Jupiter's Magnetospheric Injections
DOI: 10.1029/2018JA025708 Bibcode: 2018JGRA..123.8489D

Roussos, E.; Paranicas, C.; Bonfond, B. +3 more

Auroral emissions equatorward of the main emission at Jupiter are suggested to reflect the dynamics of the plasma in the middle magnetosphere. Here we examine the motion of the auroral signatures of magnetospheric injections appearing in Hubble Space Telescope (HST) images. Our results suggest that the injected plasma moves planetward and lags beh…

2018 Journal of Geophysical Research (Space Physics)
eHST 13
Reverse Current Model for Coronal Mass Ejection Cavity Formation
DOI: 10.3847/2041-8213/aad33c Bibcode: 2018ApJ...862L..15H

Li, Hui; Haw, Magnus A.; Wongwaitayakornkul, Pakorn +1 more

We report here a new model for explaining the three-part structure of coronal mass ejections (CMEs). The model proposes that the cavity in a CME forms because a rising electric current in the core prominence induces an oppositely directed electric current in the background plasma; this eddy current is required to satisfy the frozen-in magnetic flu…

2018 The Astrophysical Journal
SOHO 13
Is Kasei Valles (Mars) the largest volcanic channel in the solar system?
DOI: 10.1016/j.icarus.2017.10.007 Bibcode: 2018Icar..301...37L

Leverington, David W.

With a length of more than 2000 km and widths of up to several hundred kilometers, Kasei Valles is the largest outflow system on Mars. Superficially, the scabland-like character of Kasei Valles is evocative of terrestrial systems carved by catastrophic aqueous floods, and the system is widely interpreted as a product of outbursts from aquifers. Ho…

2018 Icarus
MEx 13
Coloring Jupiter's clouds: Radiolysis of ammonium hydrosulfide (NH4SH)
DOI: 10.1016/j.icarus.2017.10.041 Bibcode: 2018Icar..302..418L

Hudson, Reggie L.; Loeffler, Mark J.

Here we present our recent studies on the color and spectral reflectance changes induced by ∼0.9 MeV proton irradiation of ammonium hydrosulfide, NH4SH, a compound predicted to be an important tropospheric cloud component of Jupiter and other giant planets. Ultraviolet-visible spectroscopy was used to observe and identify reaction produ…

2018 Icarus
eHST 13
Further constraints on neutron star crustal properties in the low-mass X-ray binary 1RXS J180408.9-342058
DOI: 10.1093/mnras/sty416 Bibcode: 2018MNRAS.476.2230P

Degenaar, N.; Wijnands, R.; Parikh, A. S. +2 more

We report on two new quiescent XMM-Newton observations (in addition to the earlier Swift/XRT and XMM-Newton coverage) of the cooling neutron star crust in the low-mass X-ray binary 1RXS J180408.9-342058. Its crust was heated during the ∼4.5 month accretion outburst of the source. From our quiescent observations, fitting the spectra with a neutron …

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 13
Tidal Interactions and Mergers in Intermediate-redshift EDisCS Clusters
DOI: 10.3847/1538-4357/aaeb87 Bibcode: 2018ApJ...869....6D

Moustakas, John; Aragón-Salamanca, Alfonso; Lotz, Jennifer M. +6 more

We study the fraction of tidal interactions and mergers (TIMs) with well-identified observability timescales (f TIM) in group, cluster, and accompanying field galaxies and its dependence on redshift (z), cluster velocity dispersion (σ), and environment analyzing Hubble Space Telescope/ACS images and catalogs from the ESO Distant Cluster…

2018 The Astrophysical Journal
eHST 13
Statistics of the polarized submillimetre emission maps from thermal dust in the turbulent, magnetized, diffuse ISM
DOI: 10.1051/0004-6361/201732128 Bibcode: 2018A&A...614A.124L

Boulanger, F.; Falgarone, E.; Ghosh, T. +4 more

Context. The interstellar medium (ISM) is now widely acknowledged to display features ascribable to magnetized turbulence. With the public release of Planck data and the current balloon-borne and ground-based experiments, the growing amount of data tracing the polarized thermal emission from Galactic dust in the submillimetre provides choice diagn…

2018 Astronomy and Astrophysics
Planck 13