Search Publications

Coronal Heating and Solar Wind Formation in Quiet Sun and Coronal Holes: A Unified Scenario
DOI: 10.3847/1538-4357/abcc6b Bibcode: 2021ApJ...908...28T

Solanki, Sami K.; Tripathi, Durgesh; Nived, V. N.

Coronal holes (CHs) are darker than the quiet Sun (QS) when observed in coronal channels. This study aims to understand the similarities and differences between CHs and QS in the transition region using the Si IV 1394 Å line, recorded by the Interface Region Imaging Spectrograph, by considering the distribution of magnetic field measured by the He…

2021 The Astrophysical Journal
IRIS 16
Mass-loss law for red giant stars in simple population globular clusters
DOI: 10.1093/mnras/stab568 Bibcode: 2021MNRAS.503..694T

Milone, A. P.; Cordoni, G.; Marino, A. F. +12 more

The amount of mass lost by stars during the red-giant branch (RGB) phase is one of the main parameters to understand and correctly model the late stages of stellar evolution. Nevertheless, a fully comprehensive knowledge of the RGB mass-loss is still missing. Galactic Globular Clusters (GCs) are ideal targets to derive empirical formulations of ma…

2021 Monthly Notices of the Royal Astronomical Society
Gaia eHST 16
Ultra-compact dwarfs beyond the centre of the Fornax galaxy cluster: hints of UCD formation in low-density environments
DOI: 10.1093/mnras/stab1118 Bibcode: 2021MNRAS.504.3580S

Janz, Joachim; Mieske, Steffen; Peletier, Reynier F. +6 more

Ultra-compact dwarf galaxies (UCDs) were serendipitously discovered by spectroscopic surveys in the Fornax cluster 20 yr ago. Nowadays, it is commonly accepted that many bright UCDs are the nuclei of galaxies that have been stripped. However, this conclusion might be driven by biased samples of UCDs in high-density environments, on which most sear…

2021 Monthly Notices of the Royal Astronomical Society
Gaia eHST 16
The Chameleon on the branches: spectral state transition and dips in NGC 247 ULX-1
DOI: 10.1093/mnras/stab2427 Bibcode: 2021MNRAS.507.5567D

Fabian, A. C.; Pinto, C.; D'Aì, A. +14 more

Soft Ultra-Luminous X-ray (ULXs) sources are a subclass of the ULXs that can switch from a supersoft spectral state, where most of the luminosity is emitted below 1 keV, to a soft spectral state with significant emission above 1 keV. In a few systems, dips have been observed. The mechanism behind this state transition and the dips nature are still…

2021 Monthly Notices of the Royal Astronomical Society
XMM-Newton 16
High precision meteor observations with the Canadian automated meteor observatory: Data reduction pipeline and application to meteoroid mechanical strength measurements
DOI: 10.1016/j.icarus.2020.114097 Bibcode: 2021Icar..35414097V

Weryk, Robert J.; Stober, Gunter; Vida, Denis +3 more

Context. The mirror tracking system of the Canadian Automated Meteor Observatory (CAMO) can track meteors in real time, providing an effective angular resolution of 1 arc second and a temporal resolution of 100 frames per second. Aims. We describe the upgraded hardware and give details of the data calibration and reduction pipeline. We investigate…

2021 Icarus
Rosetta 16
Galactic bulge millisecond pulsars shining in x rays: A γ -ray perspective
DOI: 10.1103/PhysRevD.104.043007 Bibcode: 2021PhRvD.104d3007B

Calore, Francesca; Petrucci, Pierre-Olivier; Clavel, Maïca +3 more

If the mysterious Fermi-LAT GeV γ -ray excess is due to an unresolved population of millisecond pulsars (MSP) in the Galactic bulge, one expects this very same population to shine in x rays. For the first time, we address the question of what is the sensitivity of current x-ray telescopes to an MSP population in the Galactic bulge. To this end, we…

2021 Physical Review D
Gaia 16
Origin of metals in old Milky Way halo stars based on GALAH and Gaia
DOI: 10.1093/mnras/stab1982 Bibcode: 2021MNRAS.506.5410I

Kobayashi, Chiaki; Tominaga, Nozomu; Nomoto, Ken'ichi +6 more

Stellar and supernova nucleosynthesis in the first few billion years of the cosmic history have set the scene for early structure formation in the Universe, while little is known about their nature. Making use of stellar physical parameters measured by GALAH Data Release 3 with accurate astrometry from the Gaia EDR3, we have selected ~100 old main…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 16
The long period of 3He-rich solar energetic particles measured by Solar Orbiter 2020 November 17-23
DOI: 10.1051/0004-6361/202141009 Bibcode: 2021A&A...656L..11B

Lario, D.; Maksimovic, M.; Vecchio, A. +31 more

We report observations of a relatively long period of 3He-rich solar energetic particles (SEPs) measured by Solar Orbiter. The period consists of several well-resolved ion injections. The high-resolution STEREO-A imaging observations reveal that the injections coincide with extreme ultraviolet jets and brightenings near the east limb, n…

2021 Astronomy and Astrophysics
SolarOrbiter 16
NGTS-14Ab: a Neptune-sized transiting planet in the desert
DOI: 10.1051/0004-6361/202039712 Bibcode: 2021A&A...646A.183S

Bouchy, F.; Erikson, A.; Rauer, H. +35 more

Context. The sub-Jovian, or Neptunian, desert is a previously identified region of parameter space where there is a relative dearth of intermediate-mass planets with short orbital periods.
Aims: We present the discovery of a new transiting planetary system within the Neptunian desert, NGTS-14.
Methods: Transits of NGTS-14Ab were discover…

2021 Astronomy and Astrophysics
Gaia 16
An Unexpected Whistler Wave Generation Around Dipolarization Front
DOI: 10.1029/2020JA028957 Bibcode: 2021JGRA..12628957C

Wang, Z.; Chen, L.; Zhang, Y. +8 more

Dipolarization front (DF)—a sharp boundary separating hot tenuous plasmas from cold dense plasmas—is followed by a strong Bz region, which is termed flux pileup region (FPR) or dipolarizing flux bundle (DFB). Using 9 year (2001-2009) Cluster data, we show that the FPR hosts whistler waves because of the pancake distribution of electrons…

2021 Journal of Geophysical Research (Space Physics)
Cluster 16