Search Publications

Prolonged, Weak C1.2 Flares: A Source of Protons and Electrons
DOI: 10.1134/S0016793220060067 Bibcode: 2020Ge&Ae..60..699G

Struminskii, A. B.; Grigor'eva, I. Yu.; Shakhovskaya, A. N.

Two proton events (>100 MeV; GOES, ACS SPI) associated with weak flares (C1.2, GOES class) in the soft X-ray range that occurred on November 26, 2011, and September 29, 2013, are analyzed. These events were accompanied by significant fluxes of relativistic electrons (>1 MeV; SOHO EPHIN) in the interplanetary space. The time profiles of these…

2020 Geomagnetism and Aeronomy
SOHO 2
Emission-line Data Cubes of the HH 32 Stellar Jet
DOI: 10.3847/1538-3881/abadfa Bibcode: 2020AJ....160..165H

Hartigan, Patrick; Neill, James D.; Hillenbrand, Lynne A. +5 more

We analyze data cubes of over 60 emission lines in the HH 32 stellar jet acquired with the Keck Cosmic Web Imager (KCWI). The data cover the less explored blue portion of the spectrum between 3586 and 6351 Å and have both high spectral (R ∼ 10,000) and spatial (≲1″) resolution. The study includes all three major ionization states of oxygen, three …

2020 The Astronomical Journal
Gaia eHST 2
Ionized gas in the NGC 5253 supernebula: high spatial and spectral resolution observations with the JVLA and TEXES
DOI: 10.1093/mnras/staa1819 Bibcode: 2020MNRAS.497.1675B

Beck, Sara C.; Liu, Hauyu Baobab; Ho, Paul T. P. +4 more

The youngest, closest, and most compact embedded massive star cluster known excites the supernebula in the nearby dwarf galaxy NGC 5253. It is a crucial target and test case for studying the birth and evolution of the most massive star clusters. We present observations of the ionized gas in this source with high spatial and spectral resolution. Th…

2020 Monthly Notices of the Royal Astronomical Society
eHST 2
Swift/XRT, Chandra, and XMM-Newton observations of IGR J17091-3624 as it returns into quiescence
DOI: 10.1093/mnras/staa2009 Bibcode: 2020MNRAS.497.1115P

Court, J. M. C.; Altamirano, D.; Degenaar, N. +4 more

IGR J17091-3624 is a low-mass X-ray binary (LMXB), which received wide attention from the community thanks to its similarities with the bright black hole system GRS 1915+105. Both systems exhibit a wide range of highly structured X-ray variability during outburst, with time-scales from few seconds to tens of minutes, which make them unique in the …

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 2
A Survey of Venus Shock Crossings Dominated by Kinematic Relaxation
DOI: 10.1029/2020JA028256 Bibcode: 2020JGRA..12528256P

Pope, S. A.

Collisionless shocks are one of the most effective particle accelerators in the known universe. Even low Mach number shocks could have a significant role in particle heating and acceleration. Theory suggests that kinematic collisionless relaxation, the process whereby a downstream nongyroptopic ion population becomes thermalized through collisionl…

2020 Journal of Geophysical Research (Space Physics)
VenusExpress 2
A spectroscopic, photometric, polarimetric, and radio study of the eclipsing polar UZ Fornacis: the first simultaneous SALT and MeerKAT observations
DOI: 10.1093/mnras/staa080 Bibcode: 2020MNRAS.492.4298K

Hewitt, D. M.; Pretorius, M. L.; Woudt, P. A. +17 more

We present phase-resolved spectroscopy, photometry, and circular spectropolarimetry of the eclipsing polar UZ Fornacis. Doppler tomography of the strongest emission lines using the inside-out projection revealed the presence of three emission regions: from the irradiated face of the secondary star, the ballistic stream and the threading region, an…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 2
The inner gas mass-temperature profile in the core of nearby galaxy clusters
DOI: 10.1093/mnras/staa2023 Bibcode: 2020MNRAS.497.1256L

Fabian, Andrew C.; Pinto, Ciro; Liu, Haonan

We present a mass-temperature profile of gas within the central 10 kpc of a small sample of cool core clusters. The mass of the hottest gas phases, at 1.5 and 0.7 keV, is determined from X-ray spectra from the XMM Reflection Grating Spectrometers. The masses of the partially ionized atomic and the molecular phases are obtained from published H α a…

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 2
The hydrogen Balmer lines and jump in absorption in accretion disc modelling - an ultraviolet-optical spectral analysis of the dwarf novae UZ Serpentis and CY Lyrae
DOI: 10.1093/mnras/staa1093 Bibcode: 2020MNRAS.494.5244G

Blair, William P.; Szkody, Paula; Sion, Edward M. +1 more

The spectra of disc-dominated cataclysmic variables (CVs) often deviate from the spectra of accretion disc models; in particular, the Balmer jump and absorption lines are found to be shallower in the observations than in the models. We carried out a combined ultraviolet-optical spectral analysis of two dwarf novae (DNe): UZ Ser in outburst, declin…

2020 Monthly Notices of the Royal Astronomical Society
IUE 2
Variations in Ion-Component Pressure during Dipolarization in the Near-Earth Magnetotail Plasma Sheet
DOI: 10.1134/S0016793220010090 Bibcode: 2020Ge&Ae..60...20M

Malykhin, A. Yu.; Grigorenko, E. E.; Kronberg, E. A. +1 more

The dynamics of fluxes of thermal and suprathermal H+ and O+ ions and the pressure variations of these components during 11 events of magnetic field dipolarization in the plasma sheet of the geomagnetic tail are analyzed based on Cluster satellite observations. It was found that the energy of H+ and O+ i…

2020 Geomagnetism and Aeronomy
Cluster 2
White-light solar corona structure observed by naked eye and processed images
DOI: 10.1093/mnras/staa1377 Bibcode: 2020MNRAS.495.2170R

Rušin, Vojtech; Prikryl, Paul; Prikryl, Emil A.

Light and dark adaptation and luminance contrast enhancement are well-known characteristics of human vision that allow us to observe a wide range of light intensity not fully captured in standard camera images. The naked-eye observations of total eclipses, some recorded with spectacular detail in artists' paintings, reveal structure that is consis…

2020 Monthly Notices of the Royal Astronomical Society
SOHO 2