Search Publications

Synthesis of radioactive elements in novae and supernovae and their use as a diagnostic tool
DOI: 10.1016/j.newar.2020.101606 Bibcode: 2021NewAR..9201606I

Hernanz, M.; Siegert, T.; Vink, J. +5 more

Novae and supernovae play a key role in many fields of Astrophysics and Cosmology. Despite their importance, an accurate description of which objects explode and why and how they explode is still lacking. One of the main characteristics of such explosions is that they are the main suppliers of newly synthesized chemical elements in the Galaxy. Sin…

2021 New Astronomy Reviews
Gaia INTEGRAL 2
Pitch-angle distribution of accelerated electrons in 3D current sheets with magnetic islands
DOI: 10.1051/0004-6361/202039220 Bibcode: 2021A&A...648A..51Z

Zharkova, V.; Xia, Q.


Aims: This research aims to explore variations of electron pitch-angle distributions (PADs) during spacecraft crossing of reconnecting current sheets (RCSs) with magnetic islands. Our results can benchmark the sampled characteristic features with realistic PADs derived from in situ observations.
Methods: Particle motion is simulated in 2…

2021 Astronomy and Astrophysics
Cluster 2
Planetary nebulae with UVIT: A progress report
DOI: 10.1007/s12036-021-09698-3 Bibcode: 2021JApA...42...71R

Rao, N. Kameswara; Sutaria, F.; Murthy, J. +2 more

The spectral region between 1250–3000 Å contains important spectral lines to understand the morphological structures and evolution of planetary nebulae. This is the region sampled by UVIT through various filter bands both in the continuum and in e…

2021 Journal of Astrophysics and Astronomy
eHST 2
Testing the predictions of axisymmetric distribution functions of galactic dark matter with hydrodynamical simulations
DOI: 10.1088/1475-7516/2021/08/031 Bibcode: 2021JCAP...08..031P

Lavalle, Julien; Petač, Mihael; Núñez-Castiñeyra, Arturo +1 more

Signal predictions for galactic dark matter (DM) searches often rely on assumptions regarding the DM phase-space distribution function (DF) in halos. This applies to both particle (e.g. p-wave suppressed or Sommerfeld-enhanced annihilation, scattering off atoms, etc.) and macroscopic DM candidates (e.g. microlensing of primordial black holes). As …

2021 Journal of Cosmology and Astroparticle Physics
Gaia 2
Stellar wind structures in the eclipsing binary system IGR J18027-2016
DOI: 10.1051/0004-6361/202039088 Bibcode: 2021A&A...647A..75F

García, Federico; Fogantini, Federico A.; Chaty, Sylvain +1 more

Context. IGR J18027-2016 is an obscured high-mass X-ray binary formed by a neutron star accreting from the wind of a supergiant companion with a ∼4.57 d orbital period. The source shows an asymmetric eclipse profile that remained stable across several years.
Aims: We aim to investigate the geometrical and physical properties of stellar wind s…

2021 Astronomy and Astrophysics
XMM-Newton 2
Some Features of Solar Proton Events on March 7, 2011, and on February 20, 2014
DOI: 10.1134/S0010952521040067 Bibcode: 2021CosRe..59..250V

Vlasova, N. A.; Kalegaev, V. V.; Tulupov, V. I.

The paper presents the results of studying two solar proton events—on March 7, 2011, and on February 20, 2014—which are associated with solar flares having almost the same power and located at close heliolongitudes, on the western side of the solar disk. The work was done on the basis of the experimental data obtained from the ACE spacecraft and t…

2021 Cosmic Research
SOHO 2
A Uniform Series of Low-Latitude Coronal Holes in 1973-2018
DOI: 10.1007/s11207-021-01781-w Bibcode: 2021SoPh..296...40H

Asikainen, T.; Mursula, K.; Hamada, A.

Coronal holes (CHs) are regions in the solar corona characterized by plasma density lower than in the surrounding quiet Sun. Therefore they appear dark in images of the solar atmosphere made, e.g., in extreme ultraviolet (EUV). Identifying CHs on solar images is difficult since CH boundaries are not sharp, but typically obscured by magnetic struct…

2021 Solar Physics
SOHO 2
The study of runaway candidate stars in the 30 Doradus region: Using Gaia DR2 data
DOI: 10.1016/j.newast.2020.101455 Bibcode: 2021NewA...8201455G

Gebrehiwot, Yikdem Mengesha; Teklehaimanot, Berhe Tewelde

We explore the Gaia DR2 relative proper motions of seven young, massive, OB type runaway candidate stars presented by Platais et al. (2018) in the 30 Doradus (30 Dor) region of the Large Magellanic Cloud (LMC). The stars are slow runaways in the tangential plane of the 30 Dor region with relative proper motions µ ≤ 0.4 mas yr-1 th…

2021 New Astronomy
Gaia 2
Light-toned deposit in the northeastern Hellas basin formed by terrain-conforming airfall sedimentation
DOI: 10.1016/j.icarus.2021.114356 Bibcode: 2021Icar..36014356H

Wilson, S. A.; Howard, A. D.; Morgan, A. M. +2 more

Extensive exposures of a light-toned deposit (LTD) occurs on the northeastern interior slope of the Hellas basin. This deposit is on the floors of all but the youngest craters greater than 30 km in diameter in the study region centered at 83°E and 30°S, as well as in exposures on crater interior and exterior walls, on intercrater plains, and the n…

2021 Icarus
MEx 2
Study of central intensity ratio of early-type galaxies from low-density environment
DOI: 10.1093/mnras/staa3334 Bibcode: 2021MNRAS.500.1343S

Ravikumar, C. D.; Sruthi, K.

We present correlations involving central intensity ratio (CIR) of 52 early-type galaxies, including 24 ellipticals and 28 lenticulars, selected from low-density environment in the nearby (<30 Mpc) universe. CIR is found to be negatively and significantly correlated with the mass of the central supermassive black hole, central velocity dispersi…

2021 Monthly Notices of the Royal Astronomical Society
eHST 2