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CAPOS: The bulge Cluster APOgee Survey. II. The intriguing "Sequoia" globular cluster FSR 1758
DOI: 10.1051/0004-6361/202141294 Bibcode: 2021A&A...652A.158R

Cohen, Roger E.; Beers, Timothy C.; Minniti, Dante +16 more

We present results from a study of 15 red giant members of the intermediate-metallicity globular cluster (GC) FSR 1758 using high-resolution, near-infrared spectra collected with the Apache Point Observatory Galactic Evolution Experiment II survey (APOGEE-2) that were obtained as part of CAPOS (the bulge Cluster APOgee Survey). Since its very rece…

2021 Astronomy and Astrophysics
Gaia 18
Long-term stellar activity variations and their effect on radial-velocity measurements
DOI: 10.1093/mnras/stab1183 Bibcode: 2021MNRAS.505..830C

Günther, Maximilian N.; Jenkins, James S.; Watson, Christopher A. +8 more

Long-term stellar activity variations can affect the detectability of long-period and Earth-analogue extrasolar planets. We have, for 54 stars, analysed the long-term trend of five activity indicators: log $R^{\prime }_\mathrm{{HK}}$, the cross-correlation function (CCF) bisector span, CCF full-width-at-half-maximum, CCF contrast, and the area of …

2021 Monthly Notices of the Royal Astronomical Society
Gaia 18
Long-term Coherent Timing of the Accreting Millisecond Pulsar IGR J17062-6143
DOI: 10.3847/1538-4357/abf13f Bibcode: 2021ApJ...912..120B

Bult, Peter; Malacaria, Christian; Ng, Mason +2 more

We report on a coherent timing analysis of the 163 Hz accreting millisecond X-ray pulsar IGR J17062-6143. Using data collected with the Neutron Star Interior Composition Explorer and XMM-Newton, we investigated the pulsar evolution over a time span of four years. We obtained a unique phase-coherent timing solution for the stellar spin, finding the…

2021 The Astrophysical Journal
XMM-Newton 18
Reproducing the UVJ Color Distribution of Star-forming Galaxies at 0.5 < z < 2.5 with a Geometric Model of Dust Attenuation
DOI: 10.3847/2041-8213/ac3831 Bibcode: 2021ApJ...922L..32Z

Belli, Sirio; Tacchella, Sandro; Leja, Joel +1 more

We analyze the distribution of rest-frame U - V and V - J colors for star-forming galaxies at 0.5 < z < 2.5. Using stellar population synthesis, stochastic star formation histories, and a simple prescription for the dust attenuation that accounts for the shape and inclination of galaxies, we construct a model for the distribution of galaxy c…

2021 The Astrophysical Journal
Herschel 18
Estimates of the change rate of solar mass and gravitational constant based on the dynamics of the Solar System
DOI: 10.1051/0004-6361/202039893 Bibcode: 2021A&A...647A.141P

Pitjeva, E. V.; Pitjev, N. P.; Pavlov, D. A. +1 more

The estimate of the change rate of the solar gravitational parameter d(GM)∕dt is obtained from processing modern positional observations of planets and spacecraft. Observations were processed and parameters were determined basing on the numerical planetary ephemeris EPM2019. The obtained annual decrease in solar mass M acco…

2021 Astronomy and Astrophysics
Ulysses 18
The Composition of the South Polar Cap of Mars Derived From Orbital Data
DOI: 10.1029/2020JE006730 Bibcode: 2021JGRE..12606730B

Wieczorek, M. A.; Broquet, A.; Fa, W.

The flexure of the lithosphere under stresses imposed by the geologically young south polar cap is one of the few clues we have regarding the south polar cap composition and the present-day thermal state of Mars. Here, we combine radar, gravity, and topography data with a flexural loading model to estimate the bulk density (ρ) and average real die…

2021 Journal of Geophysical Research (Planets)
MEx 18
Evolution of anisotropic turbulence in the fast and slow solar wind: Theory and Solar Orbiter measurements
DOI: 10.1051/0004-6361/202140672 Bibcode: 2021A&A...656A...6A

Fedorov, A.; Horbury, T. S.; Louarn, P. +8 more


Aims: Solar Orbiter (SolO) was launched on February 9, 2020, allowing us to study the nature of turbulence in the inner heliopshere. We investigate the evolution of anisotropic turbulence in the fast and slow solar wind in the inner heliosphere using the nearly incompressible magnetohydrodynamic (NI MHD) turbulence model and SolO measurements…

2021 Astronomy and Astrophysics
SolarOrbiter 18
Parker Solar Probe observations of He/H abundance variations in SEP events inside 0.5 au
DOI: 10.1051/0004-6361/202039299 Bibcode: 2021A&A...650A..23C

Mitchell, D. G.; McComas, D. J.; Bale, S. D. +24 more


Aims: The Parker Solar Probe (PSP) orbit provides an opportunity to study the inner heliosphere at distances closer to the Sun than previously possible. Due to the solar minimum conditions, the initial orbits of PSP yielded only a few solar energetic particle (SEP) events for study. Recently during the fifth orbit, at distances from 0.45 to 0…

2021 Astronomy and Astrophysics
SOHO 18
The distribution of open clusters in the Galaxy
DOI: 10.3389/fspas.2021.656474 Bibcode: 2021FrASS...8...62M

Monteiro, Hektor; Barros, Douglas A.; Lépine, Jacques R. D. +1 more

In this work we explore the new catalog of galactic open clusters that became available recently, containing 1750 clusters that have been re-analysed using the Gaia DR2 catalog to determine the stellar memberships. We used the young open clusters as tracers of spiral arms and determined the spiral pattern rotation speed of the Galaxy and the corot…

2021 Frontiers in Astronomy and Space Sciences
Gaia 18
Characteristics of the Basal Interface of the Martian South Polar Layered Deposits
DOI: 10.1029/2021GL093631 Bibcode: 2021GeoRL..4893631K

Plaut, Jeffrey J.; Khuller, Aditya R.

We expand on previous studies of the South Polar Layered Deposits' (SPLD) basal interface using data acquired by the Mars Advanced Radar for Subsurface and Ionospheric Sounding (MARSIS) to obtain detailed maps of elevation, topography, and reflected radar power. Using these maps, we derive the thickness (ranging from 0 to 3.7 km) and volume of the…

2021 Geophysical Research Letters
MEx 18