Search Publications

The abundance of S- and Si-bearing molecules in O-rich circumstellar envelopes of AGB stars
DOI: 10.1051/0004-6361/202037900 Bibcode: 2020A&A...641A..57M

Cernicharo, J.; Agúndez, M.; Velilla-Prieto, L. +1 more


Aims: We aim to determine the abundances of SiO, CS, SiS, SO, and SO2 in a large sample of oxygen-rich asymptotic giant branch (AGB) envelopes covering a wide range of mass loss rates to investigate the potential role that these molecules could play in the formation of dust in these environments.
Methods: We surveyed a sample …

2020 Astronomy and Astrophysics
Gaia 18
Endogenic and Exogenic Contributions to Visible-wavelength Spectra of Europa's Trailing Hemisphere
DOI: 10.3847/1538-3881/abc34c Bibcode: 2020AJ....160..282T

Brown, Michael E.; Hand, Kevin P.; Trumbo, Samantha K.

The composition of Europa's trailing hemisphere reflects the combined influences of endogenous geologic resurfacing and exogenous sulfur radiolysis. Using spatially resolved visible-wavelength spectra of Europa obtained with the Hubble Space Telescope, we map multiple spectral features across the trailing hemisphere and compare their geographies w…

2020 The Astronomical Journal
eHST 18
A spectroscopic test of the rotational modulation origin of periodic Kepler photometric variability of A-type stars
DOI: 10.1093/mnras/staa2444 Bibcode: 2020MNRAS.498.2456S

Wade, G. A.; Sikora, J.; Rowe, J.

High-precision space-based photometry obtained by the Kepler and TESS missions has revealed evidence of rotational modulation associated with main-sequence (MS) A- and late B-type stars. Generally, such variability in these objects is attributed to inhomogeneous surface structures (e.g. chemical spots), which are typically linked to strong magneti…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 18
Activity and differential rotation of the early M dwarf Kepler-45 from transit mapping
DOI: 10.1093/mnras/staa103 Bibcode: 2020MNRAS.492.5141Z

Marsden, S. C.; Carter, B. D.; Valio, A. +1 more

Little is known of the activity and differential rotation of low luminosity, early M dwarfs from direct observation. We present the first stellar activity analysis of star-spots and faculae for the hot Jupiter hosting M1V dwarf Kepler-45 from Kepler transit light curves. We find star-spot and facula temperatures contrasting a few hundred degrees w…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 18
Braking indices of young radio pulsars: theoretical perspective
DOI: 10.1093/mnras/staa3070 Bibcode: 2020MNRAS.499.2826I

Igoshev, Andrei P.; Popov, Sergei B.

Recently, Parthsarathy et al. analysed long-term timing observations of 85 young radio pulsars. They found that 15 objects have absolute values of braking indices ranging ∼10-3000, far from the classical value n = 3. They also noted a mild correlation between measured value of n and characteristic age of a radio pulsar. In this article, we systema…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 18
From birth associations to field stars: mapping the small-scale orbit distribution in the Galactic disc
DOI: 10.1093/mnras/staa1358 Bibcode: 2020MNRAS.495.4098C

Xiang, Maosheng; Rix, Hans-Walter; El-Badry, Kareem +3 more

Stars born at the same time in the same place should have formed from gas of the same element composition. But most stars subsequently disperse from their birth siblings, in orbit and orbital phase, becoming 'field stars'. Here, we explore and provide direct observational evidence for this process in the Milky Way disc, by quantifying the probabil…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 18
The Influence of Varying Spacecraft Potentials and Debye Lengths on In Situ Low-Energy Ion Measurements
DOI: 10.1029/2020JA027870 Bibcode: 2020JGRA..12527870B

Stenberg Wieser, Gabriella; Wieser, Martin; Eriksson, Anders +2 more

Low-energy ions are difficult to measure, mainly due to spacecraft charging. The ions are attracted to or repelled from the charged surface prior to detection, which changes both the energy and travel direction of the ions. This results in distortions of the data, and the changed travel directions distort the effective field of view (FOV) of the i…

2020 Journal of Geophysical Research (Space Physics)
Rosetta 18
Characteristics of solar wind suprathermal halo electrons
DOI: 10.1051/0004-6361/202038830 Bibcode: 2020A&A...642A.130L

Fichtner, H.; Pierrard, V.; Lazar, M. +1 more

A suprathermal halo population of electrons is ubiquitous in space plasmas, as evidence of their departure from thermal equilibrium even in the absence of anisotropies. The origin, properties, and implications of this population, however, are poorly known. We provide a comprehensive description of solar wind halo electrons in the ecliptic, contras…

2020 Astronomy and Astrophysics
Cluster Ulysses 18
SCExAO/CHARIS Near-infrared Integral Field Spectroscopy of the HD 15115 Debris Disk
DOI: 10.3847/1538-3881/ababa6 Bibcode: 2020AJ....160..163L

Henning, Thomas; Currie, Thayne; Schneider, Glenn +23 more

We present new, near-infrared (1.1-2.4 µm) high-contrast imaging of the debris disk around HD 15115 with the Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) system coupled with the Coronagraphic High Angular Resolution Imaging Spectrograph (CHARIS). The SCExAO/CHARIS resolves the disk down to ρ ∼ 0"2 (rproj ∼ 10 au), a facto…

2020 The Astronomical Journal
Gaia eHST 18
Hubble Space Telescope Imaging of Antlia B: Star Formation History and a New Tip of the Red Giant Branch Distance
DOI: 10.3847/1538-4357/ab58d2 Bibcode: 2020ApJ...888...31H

Carlin, J. L.; Dolphin, A. E.; Crnojević, D. +8 more

A census of the satellite population around dwarf galaxy primary hosts in environments outside the Local Group is essential to understanding Λ cold dark matter galaxy formation and evolution on the smallest scales. We present deep optical Hubble Space Telescope imaging of the gas-rich, faint dwarf galaxy Antlia B (M V = -9.4)—a likely…

2020 The Astrophysical Journal
eHST 18