Search Publications

Occurrence and Architecture of Kepler Planetary Systems as Functions of Stellar Mass and Effective Temperature
DOI: 10.3847/1538-3881/ab7373 Bibcode: 2020AJ....159..164Y

Zhou, Ji-Lin; Xie, Ji-Wei; Yang, Jia-Yi

The Kepler mission has discovered thousands of exoplanets around various stars with different spectral types (M, K, G, and F) and thus different masses and effective temperatures. Previous studies have shown that the planet occurrence rate, in terms of the average number of planets per star, drops with increasing stellar effective temperature (T

2020 The Astronomical Journal
Gaia 61
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
Time-delay cosmographic forecasts with strong lensing and JWST stellar kinematics
DOI: 10.1093/mnras/staa498 Bibcode: 2020MNRAS.493.4783Y

Suyu, Sherry H.; Yıldırım, Akın; Halkola, Aleksi

We present a joint strong lensing and stellar dynamical framework for future time-delay cosmography purposes. Based on a pixelated source reconstruction and the axisymmetric Jeans equations, we are capable of constraining cosmological distances and hence the current expansion rate of the Universe (H0) to the few per cent level per lens,…

2020 Monthly Notices of the Royal Astronomical Society
eHST 61
HADES RV programme with HARPS-N at TNG. XII. The abundance signature of M dwarf stars with planets
DOI: 10.1051/0004-6361/202039478 Bibcode: 2020A&A...644A..68M

Baratella, M.; Rebolo, R.; Ribas, I. +27 more

Context. Most of our current knowledge on planet formation is still based on the analysis of main sequence, solar-type stars. Conversely, detailed chemical studies of large samples of M dwarfs hosting planets are still missing.
Aims: Correlations exist between the presence of different types of planets around FGK stars and metallicity, indivi…

2020 Astronomy and Astrophysics
Gaia 61
Magnetic Reconnection during the Post-impulsive Phase of a Long-duration Solar Flare: Bidirectional Outflows as a Cause of Microwave and X-Ray Bursts
DOI: 10.3847/1538-4357/aba8a6 Bibcode: 2020ApJ...900...17Y

Reeves, Katharine K.; Chen, Bin; Yu, Sijie +5 more

Magnetic reconnection plays a crucial role in powering solar flares, production of energetic particles, and plasma heating. However, where the magnetic reconnections occur, how and where the released magnetic energy is transported, and how it is converted to other forms remain unclear. Here we report recurring bidirectional plasma outflows located…

2020 The Astrophysical Journal
SOHO 61
The gas production of 14 species from comet 67P/Churyumov-Gerasimenko based on DFMS/COPS data from 2014 to 2016
DOI: 10.1093/mnras/staa2643 Bibcode: 2020MNRAS.498.3995L

Altwegg, Kathrin; Rubin, Martin; Läuter, Matthias +1 more

The coma of comet 67P/Churyumov-Gerasimenko has been probed by the Rosetta spacecraft and shows a variety of different molecules. The ROSINA COmet Pressure Sensor and the Double Focusing Mass Spectrometer provide in situ densities for many volatile compounds including the 14 gas species H2O, CO2, CO, H2S, O2

2020 Monthly Notices of the Royal Astronomical Society
Rosetta 60
Rationale for BepiColombo Studies of Mercury's Surface and Composition
DOI: 10.1007/s11214-020-00694-7 Bibcode: 2020SSRv..216...66R

Muinonen, Karri; Wurz, Peter; Massironi, Matteo +63 more

BepiColombo has a larger and in many ways more capable suite of instruments relevant for determination of the topographic, physical, chemical and mineralogical properties of Mercury's surface than the suite carried by NASA's MESSENGER spacecraft. Moreover, BepiColombo's data rate is substantially higher. This equips it to confirm, elaborate upon, …

2020 Space Science Reviews
BepiColombo 60
Systematic Phase Curve Study of Known Transiting Systems from Year One of the TESS Mission
DOI: 10.3847/1538-3881/ababad Bibcode: 2020AJ....160..155W

Latham, David W.; Kane, Stephen R.; Fetherolf, Tara +14 more

We present a systematic phase curve analysis of known transiting systems observed by the Transiting Exoplanet Survey Satellite (TESS) during year one of the primary mission. Using theoretical predictions for the amplitude of the planetary longitudinal atmospheric brightness modulation, stellar ellipsoidal distortion and Doppler boosting, as well a…

2020 The Astronomical Journal
Hipparcos 60
A Flare-type IV Burst Event from Proxima Centauri and Implications for Space Weather
DOI: 10.3847/1538-4357/abca90 Bibcode: 2020ApJ...905...23Z

Kaplan, David L.; Cairns, Iver H.; Lenc, Emil +10 more

Studies of solar radio bursts play an important role in understanding the dynamics and acceleration processes behind solar space weather events, and the influence of solar magnetic activity on solar system planets. Similar low-frequency bursts detected from active M-dwarfs are expected to probe their space weather environments and therefore the ha…

2020 The Astrophysical Journal
Gaia 60
The Next Generation Virgo Cluster Survey (NGVS). XIV. The Discovery of Low-mass Galaxies and a New Galaxy Catalog in the Core of the Virgo Cluster
DOI: 10.3847/1538-4357/ab339f Bibcode: 2020ApJ...890..128F

Jordán, Andrés; Zhang, Hongxin; Emsellem, Eric +28 more

The Next Generation Virgo Cluster Survey (NGVS) was designed to provide a deep census of baryonic structures in the Virgo cluster. The survey covers the 104 deg2 area from the core of Virgo out to one virial radius, in the u*griz bandpasses, to a point-source depth of g ∼ 25.9 mag (10σ) and a single pixel surface brightness limit of &mi…

2020 The Astrophysical Journal
eHST 60