Search Publications

The Host Galaxies of Tidal Disruption Events
DOI: 10.1007/s11214-020-00657-y Bibcode: 2020SSRv..216...32F

Zabludoff, Ann I.; French, K. Decker; Graur, Or +2 more

Recent studies of Tidal Disruption Events (TDEs) have revealed unexpected correlations between the TDE rate and the large-scale properties of the host galaxies. In this review, we present the host galaxy properties of all TDE candidates known to date and quantify their distributions. We consider throughout the differences between observationally-i…

2020 Space Science Reviews
eHST 102
Atmospheric Dynamics of Hot Giant Planets and Brown Dwarfs
DOI: 10.1007/s11214-020-00758-8 Bibcode: 2020SSRv..216..139S

Showman, Adam P.; Parmentier, Vivien; Tan, Xianyu

Groundbased and spacecraft telescopic observations, combined with an intensive modeling effort, have greatly enhanced our understanding of hot giant planets and brown dwarfs over the past ten years. Although these objects are all fluid, hydrogen worlds with stratified atmospheres overlying convective interiors, they exhibit an impressive diversity…

2020 Space Science Reviews
eHST 99
X-Ray Properties of TDEs
DOI: 10.1007/s11214-020-00708-4 Bibcode: 2020SSRv..216...85S

Komossa, S.; Jonker, P. G.; Auchettl, K. +1 more

Observational astronomy of tidal disruption events (TDEs) began with the detection of X-ray flares from quiescent galaxies during the ROSAT all-sky survey of 1990-1991. The flares complied with theoretical expectations, having high peak luminosities (Lx up to ≥4 ×1044erg/s), a thermal spectrum with k T ∼few×105K, a…

2020 Space Science Reviews
XMM-Newton 90
Diffuse and Pulsating Aurora
DOI: 10.1007/s11214-019-0629-3 Bibcode: 2020SSRv..216....4N

Miyoshi, Yoshizumi; Nishimura, Yukitoshi; Katoh, Yuto +14 more

This chapter reviews fundamental properties and recent advances of diffuse and pulsating aurora. Diffuse and pulsating aurora often occurs on closed field lines and involves energetic electron precipitation by wave-particle interaction. After summarizing the definition, large-scale morphology, types of pulsation, and driving processes, we review o…

2020 Space Science Reviews
Cluster 83
Dust-to-Gas and Refractory-to-Ice Mass Ratios of Comet 67P/Churyumov-Gerasimenko from Rosetta Observations
DOI: 10.1007/s11214-020-00662-1 Bibcode: 2020SSRv..216...44C

Pätzold, Martin; Choukroun, Mathieu; Thomas, Nicolas +9 more

This chapter reviews the estimates of the dust-to-gas and refractory-to-ice mass ratios derived from Rosetta measurements in the lost materials and the nucleus of 67P/Churyumov-Gerasimenko, respectively. First, the measurements by Rosetta instruments are described, as well as relevant characteristics of 67P. The complex picture of the activity of …

2020 Space Science Reviews
Rosetta 79
Investigating Mercury's Environment with the Two-Spacecraft BepiColombo Mission
DOI: 10.1007/s11214-020-00712-8 Bibcode: 2020SSRv..216...93M

André, N.; Kallio, E.; Barabash, S. +76 more

The ESA-JAXA BepiColombo mission will provide simultaneous measurements from two spacecraft, offering an unprecedented opportunity to investigate magnetospheric and exospheric dynamics at Mercury as well as their interactions with the solar wind, radiation, and interplanetary dust. Many scientific instruments onboard the two spacecraft will be com…

2020 Space Science Reviews
BepiColombo 78
Photogeologic Map of the Perseverance Rover Field Site in Jezero Crater Constructed by the Mars 2020 Science Team
DOI: 10.1007/s11214-020-00739-x Bibcode: 2020SSRv..216..127S

Liu, Yang; Mangold, Nicolas; Johnson, Jeffrey R. +64 more

The Mars 2020 Perseverance rover landing site is located within Jezero crater, a ∼50 km diameter impact crater interpreted to be a Noachian-aged lake basin inside the western edge of the Isidis impact structure. Jezero hosts remnants of a fluvial delta, inlet and outlet valleys, and infill deposits containing diverse carbonate, mafic, and hydrated…

2020 Space Science Reviews
MEx 77
Perpendicular Transport of Energetic Particles in Magnetic Turbulence
DOI: 10.1007/s11214-020-0644-4 Bibcode: 2020SSRv..216...23S

Shalchi, Andreas

Scientists have explored how energetic particles such as solar energetic particles and cosmic rays move through a magnetized plasma such as the interplanetary and interstellar medium since more than five decades. From a theoretical point of view, this topic is difficult because the particles experience complicated interactions with turbulent magne…

2020 Space Science Reviews
Ulysses 74
SIMBIO-SYS: Scientific Cameras and Spectrometer for the BepiColombo Mission
DOI: 10.1007/s11214-020-00704-8 Bibcode: 2020SSRv..216...75C

Langevin, Y.; Poulet, F.; Jorda, L. +93 more

The SIMBIO-SYS (Spectrometer and Imaging for MPO BepiColombo Integrated Observatory SYStem) is a complex instrument suite part of the scientific payload of the Mercury Planetary Orbiter for the BepiColombo mission, the last of the cornerstone missions of the European Space Agency (ESA) Horizon + science program.

2020 Space Science Reviews
BepiColombo 69
A Review of Possible Planetary Atmospheres in the TRAPPIST-1 System
DOI: 10.1007/s11214-020-00719-1 Bibcode: 2020SSRv..216..100T

Demory, Brice-Olivier; Leconte, Jérémy; Turbet, Martin +4 more

TRAPPIST-1 is a fantastic nearby (∼39.14 light years) planetary system made of at least seven transiting terrestrial-size, terrestrial-mass planets all receiving a moderate amount of irradiation. To date, this is the most observationally favourable system of potentially habitable planets known to exist. Since the announcement of the discovery of t…

2020 Space Science Reviews
eHST 61