Search Publications

The Impact of Stellar Clustering on the Observed Multiplicity and Orbital Periods of Planetary Systems
DOI: 10.3847/2041-8213/abeb22 Bibcode: 2021ApJ...911L..16L

Kruijssen, J. M. Diederik; Longmore, Steven N.; Chevance, Mélanie

It has recently been shown that stellar clustering plays an important role in shaping the properties of planetary systems. We investigate how the multiplicity distributions and orbital periods of planetary systems depend on the 6D phase space density of stars surrounding planet host systems. We find that stars in high stellar phase space density e…

2021 The Astrophysical Journal
Gaia 21
Physical and chemical structure of the Serpens filament: Fast formation and gravity-driven accretion
DOI: 10.1051/0004-6361/202039465 Bibcode: 2021A&A...646A.170G

Menten, K. M.; Belloche, A.; Henkel, C. +5 more

Context. The Serpens filament, a prominent elongated structure in a relatively nearby molecular cloud, is believed to be at an early evolutionary stage, so studying its physical and chemical properties can shed light on filament formation and early evolution.
Aims: The main goal is to address the physical and chemical properties as well as th…

2021 Astronomy and Astrophysics
Herschel 21
Predicting the Magnetic Fields of a Stealth CME Detected by Parker Solar Probe at 0.5 au
DOI: 10.3847/1538-4357/ac25f4 Bibcode: 2021ApJ...920...65P

Al-Haddad, Nada; Lynch, Benjamin J.; Palmerio, Erika +5 more

Stealth coronal mass ejections (CMEs) are eruptions from the Sun that are not associated with appreciable low-coronal signatures. Because they often cannot be linked to a well-defined source region on the Sun, analysis of their initial magnetic configuration and eruption dynamics is particularly problematic. In this article, we address this issue …

2021 The Astrophysical Journal
SOHO 21
ExoMars TGO/NOMAD-UVIS Vertical Profiles of Ozone: 1. Seasonal Variation and Comparison to Water
DOI: 10.1029/2021JE006837 Bibcode: 2021JGRE..12606837P

Aoki, S.; Vandaele, A. C.; Daerden, F. +23 more

We present ∼1.5 Mars Years (MY) of ozone vertical profiles, covering LS = 163° in MY34 to LS = 320° in MY35, a period which includes the 2018 global dust storm. Since April 2018, the Ultraviolet and Visible Spectrometer channel of the Nadir and Occultation for Mars Discovery (NOMAD) instrument aboard the ExoMars Trace Gas Orb…

2021 Journal of Geophysical Research (Planets)
ExoMars-16 21
3D core kinematics of NGC 6362: central rotation in a dynamically evolved globular cluster
DOI: 10.1093/mnras/stab1257 Bibcode: 2021MNRAS.506..813D

Vesperini, Enrico; Dalessandro, Emanuele; Kamann, Sebastian +4 more

We present a detailed 3D kinematic analysis of the central regions (R < 30 arcsec) of the low mass and dynamically evolved galactic globular cluster (GC) NGC 6362. The study is based on data obtained with ESO-VLT/MUSE used in combination with the adaptive optics module and providing ~3000 line-of-sight radial velocities, which have been complem…

2021 Monthly Notices of the Royal Astronomical Society
Gaia eHST 21
Evolution of Interplanetary Coronal Mass Ejection Complexity: A Numerical Study through a Swarm of Simulated Spacecraft
DOI: 10.3847/2041-8213/ac0d58 Bibcode: 2021ApJ...916L..15S

Poedts, Stefaan; Lugaz, Noé; Scolini, Camilla +1 more

In-situ measurements carried out by spacecraft in radial alignment are critical to advance our knowledge on the evolutionary behavior of coronal mass ejections (CMEs) and their magnetic structures during propagation through interplanetary space. Yet, the scarcity of radially aligned CME crossings restricts investigations on the evolution of CME ma…

2021 The Astrophysical Journal
SolarOrbiter 21
Discovery of Four New Clusters in the Cygnus Cloud
DOI: 10.1088/1674-4527/21/2/45 Bibcode: 2021RAA....21...45Q

Chen, Li; Zhong, Jing; Li, Jing +1 more

We report the discovery of four new open clusters (named QC 1, QC 2, QC 3 and QC 4) in the direction of Cygnus Cloud and select their members based on five astrometric parameters (l, b, ϖ, ${\mu }_{\alpha }^{* }$ , µδ) of Gaia DR2. We also derive their astrophysical parameters for each new cluster. Structure parameters are generat…

2021 Research in Astronomy and Astrophysics
Gaia 20
3He-rich solar energetic particle events observed on the first perihelion pass of Solar Orbiter
DOI: 10.1051/0004-6361/202039752 Bibcode: 2021A&A...656L...1M

Lario, D.; Rodríguez-Pacheco, J.; Wimmer-Schweingruber, R. F. +19 more

We report observations of five impulsive solar energetic particle (SEP) events observed inside 1 au during the first perihelion pass of the Solar Orbiter mission, which was launched in February 2020. These small events were all reasonably associated with active regions observed from Earth but which had rotated out of view by the time of the Solar …

2021 Astronomy and Astrophysics
SolarOrbiter 20
Rise of the Titans: Gas Excitation and Feedback in a Binary Hyperluminous Dusty Starburst Galaxy at z ∼ 6
DOI: 10.3847/1538-4357/abcf2e Bibcode: 2021ApJ...907...62R

Burgarella, Denis; Clements, David L.; Oliver, Seb +8 more

We report new observations toward the hyperluminous dusty starbursting major merger ADFS-27 (z = 5.655), using the Australia Telescope Compact Array (ATCA) and the Atacama Large Millimeter/submillimeter Array (ALMA). We detect CO (J = 2 → 1), CO (J = 8 → 7), CO (J = 9 → 8), CO (J = 10 → 9), and H2O (312 → 221) emis…

2021 The Astrophysical Journal
Gaia Herschel eHST 20
D/H in the refractory organics of comet 67P/Churyumov-Gerasimenko measured by Rosetta/COSIMA
DOI: 10.1093/mnras/stab1028 Bibcode: 2021MNRAS.504.4940P

Hilchenbach, M.; Merouane, S.; Engrand, C. +11 more

The D/H ratio is a clue to the origin and evolution of hydrogen-bearing chemical species in Solar system materials. D/H has been observed in the coma of many comets, but most such measurements have been for gaseous water. We present the first in situ measurements of the D/H ratios in the organic refractory component of cometary dust particles coll…

2021 Monthly Notices of the Royal Astronomical Society
Rosetta 20