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Understanding the rotational variability of K2 targets. HgMn star KIC 250152017 and blue horizontal branch star KIC 249660366
DOI: 10.1051/0004-6361/202037953 Bibcode: 2020A&A...639A...8K

Fossati, L.; Skarka, M.; Krtička, J. +6 more

Context. Ultraprecise space photometry enables us to reveal light variability even in stars that were previously deemed constant. A large group of such stars show variations that may be rotationally modulated. This type of light variability is of special interest because it provides precise estimates of rotational rates.
Aims: We aim to under…

2020 Astronomy and Astrophysics
Gaia 5
A Newtonian Model for the WASP-148 Exoplanetary System Enhanced with TESS and Ground-based Photometric Observations
DOI: 10.32023/0001-5237/70.3.3 Bibcode: 2020AcA....70..203M

Fernández, M.; Maciejewski, G.; Sota, A. +1 more

The WASP-148 planetary system has a rare architecture with a transiting Saturn-mass planet on a tight orbit which is accompanied by a slightly more massive planet on a nearby outer orbit. Using new space-born photometry and ground-based follow-up transit observations and data available in literature, we performed modeling that accounts for gravita…

2020 Acta Astronomica
Gaia 5
Unveiling Vela - variability of interstellar lines in the direction of the Vela supernova remnant - III. Na D and Ca II K
DOI: 10.1093/mnras/staa231 Bibcode: 2020MNRAS.493..497K

Muneer, S.; Lambert, David L.; Reddy, Arumalla B. S. +4 more

High-resolution optical spectra were obtained in 2017-2019 with The Southern African Large Telescope of 15 stars in the direction of the Vela supernova remnant. Interstellar Ca II H & K and Na I D lines are discussed in this paper. In particular, the line profiles are compared with profiles at a comparable spectral resolution obtained in 1993-…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 5
Investigation of target property effects on crater populations in long lava flows: A study in the Cerberus region, Mars, with implications for magma source identification
DOI: 10.1016/j.icarus.2019.113388 Bibcode: 2020Icar..33513388G

Burr, Devon M.; Kattenhorn, Simon A.; Golder, Keenan B.

Young volcanism on Mars is exemplified within the Cerberus region, which enables examination of relatively pristine lava flow surfaces. In this investigation, we derived model ages within the circum-Cerberus channelized lavas for sites proximal, medial, and distal to the lava flow sources, finding that these ages decrease with increasing distance …

2020 Icarus
MEx 5
The detection of solid phosphorus and fluorine in the dust from the coma of comet 67P/Churyumov-Gerasimenko
DOI: 10.1093/mnras/staa2950 Bibcode: 2020MNRAS.499.1870G

Cottin, Hervé; Fray, Nicolas; Bardyn, Anaïs +8 more

Here, we report the detection of phosphorus and fluorine in solid particles collected from the inner coma of comet 67P/Churyumov-Gerasimenko measured with the COmetary Secondary Ion Mass Analyser (COSIMA) instrument on-board the Rosetta spacecraft, only a few kilometers away from the comet nucleus. We have detected phosphorus-containing minerals f…

2020 Monthly Notices of the Royal Astronomical Society
Rosetta 5
A Catalog of Solar Flare Events Observed by the SOHO/EIT
DOI: 10.3847/1538-4365/ab9a42 Bibcode: 2020ApJS..249...20R

Martens, Petrus C. H.; Rotti, Sumanth A.; Aydin, Berkay

We have compiled a catalog of solar flares (SFs) as observed by the Extreme ultraviolet Imaging Telescope (EIT) on board the Solar and Heliospheric Observatory (SOHO) spacecraft and the Geostationary Operational Environmental Satellites (GOES) spacecraft over a span from 1997 to 2010. During mid-1998, the cadence of EIT images was revised from two…

2020 The Astrophysical Journal Supplement Series
SOHO 5
Smoothed particle inference analysis and abundance calculations of DEM L71, and comparison to SN explosion models
DOI: 10.1002/asna.202023773 Bibcode: 2020AN....341..163S

Burrows, David N.; Dwarkadas, Vikram V.; Siegel, Jared +2 more

We analyze the X‑ray emission from the supernova remnant DEM L71 using the smoothed particle inference (SPI) technique. The high Fe abundance found appears to confirm the Type Ia origin. Our method allows the separation of the material ejected in the supernova explosion from the material swept up by the supernova shock wave. We are able to calcula…

2020 Astronomische Nachrichten
XMM-Newton 5
Polytropic Index of the Solar Wind Ions Near the Earth Calculated Using a Homogeneous Magnetohydrodynamic Bernoulli Integral
DOI: 10.3847/1538-4357/abc24d Bibcode: 2020ApJ...904..167P

Wang, Xin; Pang, Xuexia; Wang, Feida +5 more

This paper, using the data of Cluster during 2001-2010, studies the polytropic processes of solar wind ions near the Earth. We calculate the polytropic index of ions for different outward electromagnetic energy ratios δE×B and entropy parameter changes δentropy based on the approach of the homogeneous magnetohydrodynamic Bern…

2020 The Astrophysical Journal
Cluster 5
Eclipsing binary XZ CMi in a hierarchical quadruple system
DOI: 10.1088/1674-4527/20/8/133 Bibcode: 2020RAA....20..133W

Zhu, Li-Ying; Wang, Zhi-Hua

The new complete BVRcIc light curves and spectra of the short-period eclipsing binary XZ CMi are presented. The results from the combined analysis based on the photometric and spectroscopic data show that XZ CMi is a near contact binary with the secondary component filling its critical Roche lobe while the primary filling 91%…

2020 Research in Astronomy and Astrophysics
Gaia 5
Long-Term Evolution of the Solar Corona Using PROBA2 Data
DOI: 10.1007/s11207-020-01635-x Bibcode: 2020SoPh..295...66M

Berghmans, David; West, Matthew J.; Mierla, Marilena +5 more

We use The Sun Watcher with Active Pixel System detector and Image Processing (SWAP) imager onboard the Project for Onboard Autonomy 2 (PROBA2) mission to study the evolution of large-scale EUV structures in the solar corona observed throughout Solar Cycle 24 (from 2010 to 2019). We discuss the evolution of the on-disk coronal features and at diff…

2020 Solar Physics
PROBA-2 5