Search Publications

Near-term interstellar probe: First step
DOI: 10.1016/j.actaastro.2019.06.013 Bibcode: 2019AcAau.162..284M

Wimmer-Schweingruber, Robert F.; McNutt, Ralph L.; Gruntman, Mike +9 more

Exploration of the heliosphere and the far reaches of our solar system by the Voyagers and New Horizons and near-Earth observations of the Kuiper Belt and exoplanetary systems have all profoundly changed how we view our own home in space. An Interstellar Probe escaping beyond the solar-system boundaries with new observational techniques would be a…

2019 Acta Astronautica
Ulysses 20
Quantifying the thermal Sunyaev-Zel'dovich effect and excess millimetre emission in quasar environments
DOI: 10.1093/mnras/stz2751 Bibcode: 2019MNRAS.490.2315H

Hilton, Matt; Sifón, Cristóbal; Battaglia, Nicholas +23 more

In this paper, we probe the hot, post-shock gas component of quasar-driven winds through the thermal Sunyaev-Zel'dovich (tSZ) effect. Combining data sets from the Atacama Cosmology Telescope, the Herschel Space Observatory, and the Very Large Array, we measure average spectral energy distributions of 109 829 optically selected, radio quiet quasars…

2019 Monthly Notices of the Royal Astronomical Society
Herschel 20
The effect of tides on the Sculptor dwarf spheroidal galaxy
DOI: 10.1093/mnras/stz1342 Bibcode: 2019MNRAS.487.5692I

Iorio, G.; Battaglia, G.; Sollima, A. +1 more

Dwarf spheroidal galaxies (dSphs) appear to be some of the most dark matter (DM)-dominated objects in the Universe. Their dynamical masses are commonly derived using the kinematics of stars under the assumption of equilibrium. However, these objects are satellites of massive galaxies (e.g. the Milky Way) and thus can be influenced by their tidal f…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 20
The Interplay of the Solar Wind Core and Suprathermal Electrons: A Quasilinear Approach for Firehose Instability
DOI: 10.3847/1538-4357/aaf72d Bibcode: 2019ApJ...871..237S

Lazar, M.; Poedts, S.; Yoon, P. H. +1 more

In the solar wind an equipartition of kinetic energy densities can be easily established between thermal and suprathermal electrons and the instability conditions are markedly altered by the interplay of these two populations. The new thresholds derived here for the periodic branch of firehose instability shape the limits of temperature anisotropy…

2019 The Astrophysical Journal
Cluster Ulysses 20
Transfer of Twists from a Mini-filament to Large-scale Loops by Magnetic Reconnection
DOI: 10.3847/1538-4357/ab55d7 Bibcode: 2019ApJ...887..239Y

Li, Ting; Xue, Zhike; Yan, Xiaoli +4 more

With high spatial and temporal resolution, Hα data from the New Vacuum Solar Telescope, X-ray images from the X-ray telescope on board Hinode and simultaneous observations from the Solar Dynamics Observatory, we present multiwavelength observations of the interaction between a mini-filament (MF) and its overlying large-scale active-region loops (A…

2019 The Astrophysical Journal
Hinode 20
A systematic study of Galactic infrared bubbles along the Galactic plane with AKARI and Herschel
DOI: 10.1093/pasj/psy126 Bibcode: 2019PASJ...71....6H

Oyabu, Shinki; Kaneda, Hidehiro; Ishihara, Daisuke +7 more

Galactic infrared (IR) bubbles, which have shell-like structures in the mid-IR wavelengths, are known to contain massive stars near their centers. Infrared bubbles in inner Galactic regions (|l| ≤ 65°, |b| ≤ 1°) have so far been studied well to understand the massive star formation mechanisms. In this study, we expand the research area to the whol…

2019 Publications of the Astronomical Society of Japan
AKARI Herschel 20
Spectral Evolution and Radial Dust Transport in the Prototype Young Eruptive System EX Lup
DOI: 10.3847/1538-4357/ab521d Bibcode: 2019ApJ...887..156A

Carmona, A.; Ábrahám, P.; Chen, L. +7 more

EX Lup is the prototype of a class of pre-main-sequence eruptive stars defined by their repetitive outbursts lasting several months. In 2008 January-September EX Lup underwent its historically largest outburst, brightening by about 4 mag in visual light. In previous studies we discovered ongoing silicate crystal formation in the inner disk during …

2019 The Astrophysical Journal
Gaia 20
Jovian Auroral Radio Sources Detected In Situ by Juno/Waves: Comparisons With Model Auroral Ovals and Simultaneous HST FUV Images
DOI: 10.1029/2019GL084799 Bibcode: 2019GeoRL..4611606L

Kurth, W. S.; Lamy, L.; Zarka, P. +4 more

Since the discovery of Jovian auroral radio emissions, the question arises of the source positions of the different components (broadband kilometric, hectometric, and decametric) and their association with far ultraviolet (FUV) auroral emissions. We surveyed Juno's first 15 perijoves to track local radio sources from in situ Juno/Waves measurement…

2019 Geophysical Research Letters
eHST 20
Green Peas in X-Rays
DOI: 10.3847/1538-4357/ab2b39 Bibcode: 2019ApJ...880..144S

Ehle, M.; Svoboda, J.; Orlitová, I. +1 more

Green Peas represent a population of compact, highly star-forming dwarf galaxies at redshifts z ∼ 0.2-0.3 that have recently been found to show signatures of ultraviolet ionizing radiation leakage. They are being considered as analogs to high-redshift star-forming galaxies, possibly responsible for cosmic reionization. Despite intensive studies of…

2019 The Astrophysical Journal
XMM-Newton 20
Observing the gas component of circumplanetary disks around wide-orbit planet-mass companions in the (sub)mm regime
DOI: 10.1051/0004-6361/201834899 Bibcode: 2019A&A...624A..16R

Waters, L. B. F. M.; Woitke, P.; Kamp, I. +6 more

Context. Several detections of wide-orbit planet-mass/substellar companions around young solar-like stars were reported in the last decade. The origin of those possible planets is still unclear, but accretion tracers and VLT/SPHERE observations indicate that they are surrounded by circumplanetary material or even a circumplanetary disk (CPD).

2019 Astronomy and Astrophysics
Gaia 20