Search Publications

The magnetic field clock angle departure in the Venusian magnetosheath and its response to IMF rotation
DOI: 10.1051/0004-6361/202346989 Bibcode: 2023A&A...677A.142X

Xu, Qi; Zhang, Tielong; Rong, Zhaojin +4 more

We investigate the characteristics of interplanetary magnetic field (IMF) draping in the Venusian magnetosheath using both Venus Express (VEX) observations and magnetohydrodynamics simulations. The distributions of magnetosheath field clock angle illustrate the nearly symmetric morphology of draped magnetic field with respect to the solar wind ele…

2023 Astronomy and Astrophysics
VenusExpress 3
Search for Dormant Black Holes in the OGLE Data
DOI: 10.32023/0001-5237/73.3.1 Bibcode: 2023AcA....73..197K

Mróz, P.; Kapusta, M.

Light curves of ellipsoidal variables collected by the Optical Gravitational Lensing Experiment (OGLE) were analyzed, in order to search for dormant black hole candidates. After the preselection based on the amplitude of ellipsoidal modulation, each object was investigated by means of the spectral energy distribution fit, which allowed us to selec…

2023 Acta Astronomica
Gaia XMM-Newton 3
The first evidence of tidally induced activity in a brown dwarf-M dwarf pair: a Chandra study of the NLTT 41135/41136 system
DOI: 10.1093/mnras/stad2277 Bibcode: 2023MNRAS.524.5954I

Stelzer, Beate; Poppenhaeger, Katja; Wolk, Scott J. +3 more

The magnetic activity of low-mass stars changes as they age. The primary process decreasing the stellar activity level is the angular momentum loss via magnetized stellar wind. However, processes like tidal interactions between stars and their close companions may slow down the braking effect and the subsequent decrease of the activity level. Unti…

2023 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 3
X-rays and TESS observations of symbiotic binary stars
Bibcode: 2023BAAA...64...59L

Nuñez, N. E.; Mukai, K.; Sokoloski, J. L. +5 more

Symbiotic stars are strongly interacting binaries composed of a white dwarf accreting from its red giant companion. We studied five symbiotics stars: BD~Cam, V1261~Ori, NQ~Gem, CD~-27~8661, CD~-36~8436 using observations from the Swift/XRT and XMM-Newton satellites in X-rays and from TESS in the optical. The X-ray spectra were fit with absorbed op…

2023 Boletin de la Asociacion Argentina de Astronomia La Plata Argentina
XMM-Newton 3
Insights into the interaction between defrosting seasonal ices and gully activity from CaSSIS and HiRISE observations in Sisyphi Cavi, Mars
DOI: 10.1016/j.pss.2023.105743 Bibcode: 2023P&SS..23505743P

Pajola, M.; Munaretto, G.; Vincendon, M. +10 more

Martian gullies are surface features, typically composed of an alcove, a channel and a depositional apron. They have been extensively studied since their first observations in the 2000s and were initially attributed to the action of liquid water. Later studies highlighted that their activity is spatially and temporally correlated with the seasonal…

2023 Planetary and Space Science
ExoMars-16 3
Reaching Submillisecond Accuracy in Stellar Occultations and Artificial Satellite Tracking
DOI: 10.1088/1538-3873/acacc8 Bibcode: 2023PASP..135b5001K

Kamiński, K.; Marciniak, A.; Weber, C. +2 more

In recent years, there appeared a need for astronomical observations timed with submillisecond accuracy. These include, e.g., timing stellar occultations by small, subkilometer, or fast near-Earth asteroids and tracking artificial satellites in low-Earth orbit using optical sensors. Precise astrometry of fast-moving satellites and accurate timing …

2023 Publications of the Astronomical Society of the Pacific
Gaia 3
Radio-optical Reference Catalog, Version 1
DOI: 10.3847/1538-3881/acd84c Bibcode: 2023AJ....166....8M

Secrest, Nathan J.; Makarov, Valeri V.; Johnson, Megan C.

The fundamental celestial reference frame (CRF) is based on two catalogs of astrometric positions: the third realization of the International Celestial Reference Frame (ICRF3), and the much larger Gaia CRF, built from the third data release (DR3). The objects in common between these two catalogs are mostly distant AGNs and quasars that are both su…

2023 The Astronomical Journal
Gaia 3
Cometary dust collected by MIDAS on board Rosetta. I. Dust particle catalog and statistics
DOI: 10.1051/0004-6361/202245262 Bibcode: 2023A&A...673A.129K

Bentley, M. S.; Mannel, T.; Longobardo, A. +5 more

Context. The Micro-Imaging Dust Analysis System (MIDAS) atomic force microscope (AFM) on board the Rosetta comet orbiter has been dedicated to the collection and 3D topographical investigation of cometary dust in the size range of a few hundreds of nanometers to tens of micrometers with a resolution down to a few nanometers.
Aims: We aim to c…

2023 Astronomy and Astrophysics
Rosetta 3
OMEGA/Mars Express: A new martian atmospheric dust hunter
DOI: 10.1016/j.icarus.2022.115366 Bibcode: 2023Icar..39215366L

Vincendon, Mathieu; Leseigneur, Yann

While dust is a key parameter of Mars climate, its behaviour from one year to the next can appear erratic. This variability is notably related to Global Dust Storms (GDS) which occur only certain years with different onset, duration and intensity. The interannual variabilities of the dust cycle may notably explain some characteristics of Recurring…

2023 Icarus
MEx 3
Multi-spacecraft observations of near-relativistic electron events at different radial distances
DOI: 10.1051/0004-6361/202345955 Bibcode: 2023A&A...675A.155K

Rodríguez-Pacheco, J.; Wimmer-Schweingruber, R. F.; Gómez-Herrero, R. +11 more


Aims: We study the radial evolution of near-relativistic solar energetic electron (SEE) events observed by at least two spacecraft at different heliocentric distances and with small separation angles between their magnetic footpoints at the Sun.
Methods: We identified SEE events for which Solar Orbiter and either Wind or STEREO-A had a s…

2023 Astronomy and Astrophysics
SolarOrbiter 3