Search Publications

Empirical relations between the intensities of Lyman lines of H and He+
DOI: 10.1051/0004-6361/202141960 Bibcode: 2022A&A...657A..86G

Vial, J. -C.; Auchère, F.; Bocchialini, K. +9 more

Context. Empirical relations between major UV and extreme UV spectral lines are one of the inputs for models of chromospheric and coronal spectral radiances and irradiances. They are also needed for the interpretation of some of the observations of the Solar Orbiter mission.
Aims: We aim to determine an empirical relation between the intensit…

2022 Astronomy and Astrophysics
SOHO 6
Explanation of Heliospheric Energetic Neutral Atom Fluxes Observed by the Interstellar Boundary Explorer
DOI: 10.3847/2041-8213/ac92e2 Bibcode: 2022ApJ...937L..38Z

McComas, D. J.; Rankin, J. S.; Dayeh, M. A. +3 more

Interstellar neutral atoms propagating into the heliosphere experience charge exchange with the supersonic solar wind (SW) plasma, generating ions that are picked up by the SW. These pickup ions (PUIs) constitute ~25% of the proton number density by the time they reach the heliospheric termination shock (HTS). Preferential acceleration of PUIs at …

2022 The Astrophysical Journal
Ulysses 6
1-DREAM: 1D Recovery, Extraction and Analysis of Manifolds in noisy environments
DOI: 10.1016/j.ascom.2022.100658 Bibcode: 2022A&C....4100658C

Smith, R.; Peletier, R.; Mastropietro, M. +7 more

Filamentary structures (one-dimensional manifolds) are ubiquitous in astronomical data sets. Be it in particle simulations or observations, filaments are always tracers of a perturbation in the equilibrium of the studied system and hold essential information on its history and future evolution. However, the recovery of such structures is often com…

2022 Astronomy and Computing
Gaia 6
A polarimetric study of asteroids in comet-like orbits
DOI: 10.1051/0004-6361/202142014 Bibcode: 2022A&A...658A.158G

Watanabe, Makoto; Imai, Masataka; Kim, Yoonyoung +16 more

Context. Asteroids in comet-like orbits (ACOs) consist of asteroids and dormant comets. Due to their similar appearance, it is challenging to distinguish dormant comets from ACOs via general telescopic observations. Surveys for discriminating dormant comets from the ACO population have been conducted via spectroscopy or optical and mid-infrared ph…

2022 Astronomy and Astrophysics
AKARI 6
Partially-Saturated Brines Within Basal Ice or Sediments Can Explain the Bright Basal Reflections in the South Polar Layered Deposits
DOI: 10.1029/2022JE007398 Bibcode: 2022JGRE..12707398S

Lauro, S. E.; Pettinelli, E.; Orosei, R. +5 more

Strong radar reflections have been previously mapped at the base of the Martian South Polar Layered Deposits. Here, we analyze laboratory measurements of dry and briny samples to determine the cause of this radar return. We find that liquid vein networks consisting of brines at the grain boundaries of ice crystals can greatly enhance the electrica…

2022 Journal of Geophysical Research (Planets)
MEx 6
Variations of the Internal Asymmetries of Sunspot Groups during Their Decay
DOI: 10.3847/1538-4357/ac3de6 Bibcode: 2022ApJ...925...87M

Muraközy, Judit

The aim of the present study is to show the varying asymmetries during the decay of sunspot groups. The source of input data is the SOHO/MDI-Debrecen Database sunspot catalog that contains the magnetic polarity data for time interval 1996-2010. Several types of asymmetries were examined on the selected sample of 142 sunspot groups. The leading-fol…

2022 The Astrophysical Journal
SOHO 6
Weather forecast of the Milky Way: shear and stellar feedback determine the lives of Galactic-scale filaments
DOI: 10.1093/mnrasl/slac076 Bibcode: 2022MNRAS.516L..35L

Li, Guang-Xing; Chen, Bing-Qiu; Zhou, Ji-Xuan

The interstellar medium (ISM) is an inseparable part of the Milky Way ecosystem whose evolutionary history remains a challenging question. We trace the evolution of the molecular ISM using a sample of young stellar objects (YSO) association-molecular cloud complex (YSO-MC complex). We derive their three-dimensional (3D) velocities by combining the…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 6
No Evolution in the Half-mass Radius of Milky Way-type Galaxies over the Last 10 Gyr
DOI: 10.3847/2041-8213/ac76c8 Bibcode: 2022ApJ...932L..23H

Tacchella, Sandro; Park, Minjung; Naidu, Rohan P. +3 more

The Milky Way (MW) galaxy is in focus, thanks to new observational data. Here we shed new light on the MW's past by studying the structural evolution of MW progenitors, which we identify from extragalactic surveys. Specifically, we constrain the stellar-mass growth history (SMGH) of the MW with two methods: (i) direct measurement of the MW's star …

2022 The Astrophysical Journal
eHST 6
Figures of merit for a stochastic gravitational-wave background measurement by LISA: Implications of LISA Pathfinder noise correlations
DOI: 10.1103/PhysRevD.106.063025 Bibcode: 2022PhRvD.106f3025B

Christensen, Nelson; Meyer, Renate; Boileau, Guillaume

An important goal of the Laser Interferometer Space Antenna (LISA) is to observe a stochastic gravitational-wave background (SGWB). A study of possible correlated noise in LISA is relevant to establish limits for this future measurement. To test noise investigation methods under somewhat realistic conditions, we use the data of LISA Pathfinder. We…

2022 Physical Review D
LISAPathfinder 6
Dust Evolution in the Coma of Distant, Inbound Comet C/2017 K2 (PANSTARRS)
DOI: 10.3847/PSJ/ac6d58 Bibcode: 2022PSJ.....3..135Z

Kolokolova, Ludmilla; Zhang, Qicheng; Ye, Quanzhi +1 more

C/2017 K2 (PANSTARRS) is an Oort Cloud comet previously observed to be active at heliocentric distances r > 20 au on what is likely its first passage through the inner solar system. We observed the comet on 2021 March 19-20 at r = 6.82 au preperihelion and 8.°35 phase angle with the Hubble Space Telescope (HST), and obtained high spatial resolu…

2022 The Planetary Science Journal
Gaia eHST 6