Search Publications

The Acceleration of Energetic Particles at Coronal Shocks and Emergence of a Double Power-law Feature in Particle Energy Spectra
DOI: 10.3847/1538-4357/ab3848 Bibcode: 2019ApJ...883...49K

Chen, Yao; Giacalone, Joe; Guo, Fan +1 more

We present numerical modeling of particle acceleration at coronal shocks propagating through a streamer-like magnetic field by solving the Parker transport equation with spatial diffusion both along and across the magnetic field. We show that the location on the shock where the high-energy particle intensity is the largest, depends on the energy o…

2019 The Astrophysical Journal
SOHO 24
Signs of accretion in the white dwarf + brown dwarf binary NLTT5306
DOI: 10.1093/mnras/stz127 Bibcode: 2019MNRAS.484.2566L

Maxted, P. F. L.; Page, K. L.; Wynn, G. A. +4 more

We present new XSHOOTER spectra of NLTT5306, a 0.44 ± 0.04 M white dwarf in a short period (101 min) binary system with a brown dwarf companion that is likely to have previously undergone common envelope evolution. We have confirmed the presence of H α emission and discovered Na I absorption associated with the white dwarf. These obser…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 24
Compact Star-forming Galaxies as Old Starbursts Becoming Quiescent
DOI: 10.3847/1538-4357/ab418b Bibcode: 2019ApJ...886...88G

Ivison, R. J.; Gómez-Guijarro, C.; Magdis, G. E. +8 more

Optically compact star-forming galaxies (SFGs) have been proposed as immediate progenitors of quiescent galaxies, although their origin and nature are debated. Were they formed in slow secular processes or in rapid merger-driven starbursts? Answering this question would provide fundamental insight into how quenching occurs. We explore the location…

2019 The Astrophysical Journal
eHST 24
The integrated properties of the CALIFA galaxies: model-derived galaxy parameters and quenching of star formation
DOI: 10.1093/mnras/sty2857 Bibcode: 2019MNRAS.483..370B

Zezas, A.; Ciesla, L.; Charmandaris, V. +6 more

We present a study of the integrated properties of the 835 galaxies in the Calar-Alto Legacy Integral Field spectroscopy Area survey. To derive the main physical parameters of the galaxies we have fitted their UV-to-IR spectral energy distributions (SEDs) with sets of theoretical models using CIGALE. We perform a comparison of the integrated galax…

2019 Monthly Notices of the Royal Astronomical Society
AKARI 24
Local standard of rest based on Gaia DR2 catalog
DOI: 10.1088/1674-4527/19/5/68 Bibcode: 2019RAA....19...68D

Zhu, Zi; Liu, Jia-Cheng; Ding, Ping-Jie

The local standard of rest (LSR) provides a reference framework for studies of Galactic kinematics. Determination of the LSR corresponds to the measurement of solar peculiar motion, which is under debate due to the fact that different methods and samples have been used. Adopting the astrometric data and line-of-sight velocities of main sequence st…

2019 Research in Astronomy and Astrophysics
Gaia 24
Relativistic Components of the Ultra-fast Outflow in the Quasar PDS 456 from Chandra/HETGS, NuSTAR, and XMM-Newton Observations
DOI: 10.3847/1538-4357/ab0082 Bibcode: 2019ApJ...873...29B

Danehkar, Ashkbiz; Nowak, Michael A.; Marshall, Herman L. +1 more

We present the spectral analysis of Chandra/High Energy Transmission Grating Spectrometer (HETGS) and NuSTAR observations of the quasar PDS 456 from 2015, and XMM-Newton and NuSTAR archival data from 2013 to 2014, together with Chandra/HETGS data from 2003. We analyzed these three different epochs in a consistent way, looking for absorption featur…

2019 The Astrophysical Journal
XMM-Newton 24
Search for Surviving Companions of Progenitors of Young LMC SN Ia Remnants
DOI: 10.3847/1538-4357/ab4a03 Bibcode: 2019ApJ...886...99L

Leibundgut, Bruno; Pan, Kuo-Chuan; Ricker, Paul M. +9 more

We have used two methods to search for surviving companions of Type Ia supernova progenitors in three Balmer-dominated supernova remnants in the Large Magellanic Cloud: 0519-69.0, 0505-67.9 (DEM L71), and 0548-70.4. In the first method, we use the Hubble Space Telescope photometric measurements of stars to construct color-magnitude diagrams (CMDs)…

2019 The Astrophysical Journal
eHST 24
H/C elemental ratio of the refractory organic matter in cometary particles of 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361/201834797 Bibcode: 2019A&A...630A..27I

Alexander, C.; Hilchenbach, M.; Engrand, C. +11 more

Context. Because comets are part of the most primitive bodies of our solar system, establishing their chemical composition and comparing them to other astrophysical bodies gives new constraints on the formation and evolution of organic matter throughout the solar system. For two years, the time-of-flight secondary ion mass spectrometer COmetary Se…

2019 Astronomy and Astrophysics
Rosetta 24
Comprehensive Analysis of the Formation of a Shock Wave Associated with a Coronal Mass Ejection
DOI: 10.3847/1538-4357/aaf9af Bibcode: 2019ApJ...871..212F

Susino, Roberto; Frassati, Federica; Mancuso, Salvatore +1 more

On 2014 November 1, a solar prominence eruption associated with a C2.7 class flare and a type II radio burst resulted in a fast partial halo coronal mass ejection (CME). Images acquired in the extreme ultraviolet (EUV) by the Solar Dynamics Observatory/Atmospheric Imaging Assembly (AIA) and PROBA2/SWAP and in white light (WL) by Solar and Heliosph…

2019 The Astrophysical Journal
PROBA-2 SOHO 24
An observer's view on the future of asteroseismology
DOI: 10.3389/fspas.2019.00026 Bibcode: 2019FrASS...6...26P

Paparó, Margit

Scientific research is a continuous process, and the speed of future progress can be estimated by the pace of finding explanations for previous research questions. In this observer's based view of stellar pulsation and asteroseismology, we start with the earliest observations of variable stars and the techniques used to observe them. The earliest …

2019 Frontiers in Astronomy and Space Sciences
Gaia 24