Search Publications

The multiphase environment in the centre of Centaurus A
DOI: 10.1093/mnras/staa3515 Bibcode: 2021MNRAS.500.3536B

De Marco, B.; Migliori, G.; Różańska, A. +6 more

We study the multiphase medium in the vicinity of the active galactic nucleus Centaurus A (Cen A). Combined high-resolution observations with the Atacama Large Millimeter/submillimeter Array (ALMA) and Chandra X-ray Observatory indicate that the hot X-ray emitting plasma coexists with the warm and cold media in Cen A. This complex environment is a…

2021 Monthly Notices of the Royal Astronomical Society
XMM-Newton 7
The bi-modal 7Li distribution of the Milky Way's thin-disk dwarf stars. The role of Galactic-scale events and stellar evolution
DOI: 10.1051/0004-6361/202141280 Bibcode: 2021A&A...656A..64R

Cifuentes, C.; Roca-Fàbrega, S.; Llorente de Andrés, F. +2 more

Context. The lithium abundance, A(Li), in stellar atmospheres suffers from various enhancement and depletion processes during the star's lifetime. While several studies have demonstrated that these processes are linked to the physics of stellar formation and evolution, the role that Galactic-scale events play in the galactic A(Li) evolution is not…

2021 Astronomy and Astrophysics
Gaia 7
Magnetohydrodynamic Turbulence in the Earth's Magnetotail from Observations and Global MHD Simulations
DOI: 10.3389/fspas.2021.620519 Bibcode: 2021FrASS...8...23E

Lapenta, Giovanni; Goldstein, Melvyn L.; El-Alaoui, Mostafa +2 more

Magnetohydrodynamic (MHD) turbulent flows are found in the solar wind, the magnetosheath and the magnetotail plasma sheet. In this paper, we review both observational and theoretical evidence for turbulent flow in the magnetotail. MHD simulations of the global magnetosphere for southward interplanetary magnetic field (IMF) exhibit nested vortices …

2021 Frontiers in Astronomy and Space Sciences
Cluster 7
Catalogue of in situ observed solar energetic electrons from ACE/EPAM instrument
DOI: 10.1093/mnras/stab1564 Bibcode: 2021MNRAS.505.5212S

Miteva, Rositsa; Samwel, Susan W.

We present the first comprehensive catalogue of in situ observed solar energetic electron (SEE) events that covers solar cycles [SCs] 23 and 24 in the energy range 103-315 keV. The electron enhancements are detected by the Electron, Proton, and Alpha Monitor - Deflected Electrons instrument [EPAM-DE] aboard the ACE spacecraft. Onset time, peak tim…

2021 Monthly Notices of the Royal Astronomical Society
SOHO 7
Multi-wavelength observations and modelling of a quiescent cloud LDN1512
DOI: 10.1051/0004-6361/202038401 Bibcode: 2021A&A...647A.109S

Ysard, Nathalie; Juvela, Mika; Saajasto, Mika +2 more

Context. Light scattering at near-infrared (NIR) wavelengths has been used to study the optical properties of the interstellar dust grains, but these studies are limited by the assumptions on the strength of the radiation field. On the other hand, thermal dust emission can be used to constrain the properties of the radiation field, although this i…

2021 Astronomy and Astrophysics
Gaia Herschel 7
Active Boulder Falls in Terra Sirenum, Mars: Constraints on Timing and Causes
DOI: 10.1029/2021GL094817 Bibcode: 2021GeoRL..4894817G

Conway, Susan J.; Grindrod, Peter M.; Davis, Joel M. +1 more

We use time series images to identify significant active boulder falls in an impact crater on Mars. Evidence for active boulder falls include boulder trails with impact marks from bouncing and rolling, and dark patches from boulder impacts away from the base of the crater walls. We were able to define three time periods with active boulder falls a…

2021 Geophysical Research Letters
ExoMars-16 MEx 7
From downtown to the outskirts: a radio survey of the Orion Nebula Cluster
DOI: 10.1093/mnras/stab1826 Bibcode: 2021MNRAS.506.3169V

Bally, J.; Forbrich, J.; Dzib, S. A. +1 more

We present a newly enlarged census of the compact radio population towards the Orion Nebula Cluster (ONC) using high-sensitivity continuum maps (3-10 $\mu$Jy beam-1) from a total of ~30-h centimetre-wavelength observations over an area of ~20 × 20 arcmin2 obtained in the C-band (4-8 GHz) with the Karl G. Jansky Very Large Arr…

2021 Monthly Notices of the Royal Astronomical Society
Gaia eHST 7
Towards a larger sample of radio jets from quiescent black hole X-ray binaries
DOI: 10.1093/mnras/stab644 Bibcode: 2021MNRAS.503.3784P

Maccarone, T. J.; Gandhi, P.; Miller-Jones, J. C. A. +5 more

Quiescent black hole X-ray binaries (X-ray luminosities ${\lesssim} 10^{34}\,{\rm erg}\, {\rm s}^{-1}$) are believed to be fed by hot accretion flows that launch compact, relativistic jets. However, due to their low luminosities, quiescent jets have been detected in the radio waveband from only five systems so far. Here, we present radio observati…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 7
A new method for detecting solar atmospheric gravity waves
DOI: 10.1098/rsta.2020.0178 Bibcode: 2021RSPTA.37900178C

Fleck, Bernhard; Berrilli, Francesco; Calchetti, Daniele +2 more

Internal gravity waves have been observed in the Earth's atmosphere and oceans, on Mars and Jupiter, and in the Sun's atmosphere. Despite ample evidence for the existence of propagating gravity waves in the Sun's atmosphere, we still do not have a full understanding of their characteristics and overall role for the dynamics and energetics of the s…

2021 Philosophical Transactions of the Royal Society of London Series A
Hinode SOHO 7
Quest for the Upcoming Periastron Passage of an Episodic Dust Maker and Particle-accelerating Colliding-wind Binary: WR 125
DOI: 10.3847/1538-3881/ac2506 Bibcode: 2021AJ....162..257A

Pandey, J. C.; Pandey, S. B.; Sharma, Saurabh +4 more

We have carried out a long-term infrared and X-ray investigation of the colliding-wind binary WR 125 (WC7 + O9III). The source was monitored using AstroSat Soft X-ray Telescope and the Tata Institute of Fundamental Research Near Infrared Imaging Camera-II mounted at the back of 3.6 m Devasthal Optical Telescope. WR 125 appeared brighter in the nea…

2021 The Astronomical Journal
XMM-Newton 7