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A Multiwavelength Dynamical State Analysis of ACT-CL J0019.6+0336
DOI: 10.3390/galaxies9040097 Bibcode: 2021Galax...9...97P

Hilton, Matt; Moodley, Kavilan; Wollack, Edward J. +8 more

In our study, we show a multiwavelength view of ACT-CL J0019.6+0336 (which hosts a radio halo), to investigate the cluster dynamics, morphology, and ICM. We use a combination of XMM-Newton images, Dark Energy Survey (DES) imaging and photometry, SDSS spectroscopic information, and 1.16 GHz MeerKAT data to study the cluster properties. Various X-ra…

2021 Galaxies
XMM-Newton 6
In Situ Observations of the Ion Diffusion Region in the Venusian Magnetotail
DOI: 10.1029/2020JA028547 Bibcode: 2021JGRA..12628547G

Barabash, S.; Futaana, Y.; Wei, Y. +8 more

Utilizing the in situ observations of the Analyzer of Space Plasmas and Energetic Atoms (ASPERA 4) and the magnetometer (MAG) onboard Venus Express, we report evidence of crossing the ion diffusion region of magnetic reconnection. Evidence of magnetic reconnection is based on two cases recorded by Venus Express in the Venusian magnetotail. In both…

2021 Journal of Geophysical Research (Space Physics)
VenusExpress 6
Asteroseismology of the heartbeat star KIC 5006817
DOI: 10.31577/caosp.2021.51.1.45 Bibcode: 2021CoSka..51...45M

Merc, J.; Sánchez Arias, J. P.; Beck, P. G. +2 more

This paper summarizes the project work on asteroseismology at the ERASMUS+ GATE 2020 Summer school on space satellite data. The aim was to do a global asteroseismic analysis of KIC 5006817, and quantify its stellar properties using the high-quality, state of the art space missions data. We employed the aperture photometry to analyze the data from …

2021 Contributions of the Astronomical Observatory Skalnate Pleso
Gaia 6
Ultraluminous X-ray sources in seven edge-on spiral galaxies
DOI: 10.1093/mnras/stab2850 Bibcode: 2021MNRAS.508.4008D

Kundu, Arunav; Strader, Jay; Dage, Kristen C. +8 more

We investigate a sample of seven edge-on spiral galaxies using Chandra observations. Edge-on spiral galaxies allow us to clearly separate source associated with their star-forming regions versus the outer edges of the system, offering a clear advantage over other systems. We uncover a number of X-ray point sources across these galaxies, and after …

2021 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton eHST 6
Jupiter's X-ray aurora during UV dawn storms and injections as observed by XMM-Newton, Hubble, and Hisaki
DOI: 10.1093/mnras/stab2218 Bibcode: 2021MNRAS.507.1216W

Coates, A. J.; Branduardi-Raymont, G.; Bonfond, B. +9 more

We present results from a multiwavelength observation of Jupiter's northern aurorae, carried out simultaneously by XMM-Newton, the Hubble Space Telescope (HST), and the Hisaki satellite in 2019 September. HST images captured dawn storms and injection events in the far-ultraviolet aurora several times during the observation period. Magnetic reconne…

2021 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 6
UVIT study of UV bright stars in the globular cluster NGC 4147
DOI: 10.1007/s12036-020-09687-y Bibcode: 2021JApA...42...36K

Pradhan, Ananta C.; Mohapatra, Abhisek; Kumar, Ranjan +4 more

We present far ultraviolet (FUV) observations of globular cluster NGC 4147 using three FUV filters, BaF2 (F154W), sapphire (F169M), and silica (F172M) of Ultra-Violet Imaging Telescope (UVIT) on-board the AstroSat satellite. W…

2021 Journal of Astrophysics and Astronomy
Gaia 6
Characterization of dense Planck clumps observed with Herschel and SCUBA-2
DOI: 10.1051/0004-6361/202037791 Bibcode: 2021A&A...654A.123M

Juvela, M.; Montillaud, J.; Traficante, A. +15 more

Context. Although the basic processes of star formation (SF) are known, more research is needed on SF across multiple scales and environments. The Planck all-sky survey provided a large catalog of Galactic cold clouds and clumps that have been the target of several follow-up surveys.
Aims: We aim to characterize a diverse selection of dense, …

2021 Astronomy and Astrophysics
AKARI Herschel 6
Solar Orbiter's encounter with the tail of comet C/2019 Y4 (ATLAS): Magnetic field draping and cometary pick-up ion waves
DOI: 10.1051/0004-6361/202141229 Bibcode: 2021A&A...656A..39M

Fedorov, A.; Livi, S.; Müller, D. +36 more

Context. Solar Orbiter is expected to have flown close to the tail of comet C/2019 Y4 (ATLAS) during the spacecraft's first perihelion in June 2020. Models predict a possible crossing of the comet tails by the spacecraft at a distance from the Sun of approximately 0.5 AU.
Aims: This study is aimed at identifying possible signatures of the int…

2021 Astronomy and Astrophysics
SolarOrbiter 6
The Spatial and Temporal Distribution of Nighttime Ozone and Sulfur Dioxide in the Venus Mesosphere as Deduced From SPICAV UV Stellar Occultations
DOI: 10.1029/2020JE006625 Bibcode: 2021JGRE..12606625E

Montmessin, F.; Korablev, O.; Bertaux, J. -L. +5 more

The nighttime ozone and sulfur dioxide distributions were analyzed using the entire Spectroscopy for the Investigation of the Characteristics of the Atmosphere of Venus (SPICAV) UV/Venus Express stellar occultation data set. After the discovery of an ozone layer at 100 km in the mesosphere reported by Montmessin, Bertaux, et al. (2011,

VenusExpress 6
Modelling X-ray RMS spectra II: the ultrafast outflow of PDS 456
DOI: 10.1093/mnras/staa3559 Bibcode: 2021MNRAS.500.4506H

Reeves, J. N.; Alston, W. N.; Matzeu, G. A. +6 more

We present an improved model for excess variance spectra describing ultrafast outflows and successfully apply it to the luminous ($L_{\rm bol}\sim 10^{47}\mathrm{erg}\, \mathrm{s}^{-1}$) low-redshift (z = 0.184) quasar Pico del Dias Survey (PDS) 456. The model is able to account well for the broadening of the spike-like features of these outflows …

2021 Monthly Notices of the Royal Astronomical Society
XMM-Newton 6