Search Publications

Insights from multi-wavelength observations during high and low states of non-magnetic CVs
DOI: 10.1016/j.asr.2019.07.008 Bibcode: 2020AdSpR..66.1090S

Szkody, Paula

Close binaries containing a white dwarf accreting from a disk that receives material from a late stellar companion show an interesting variety of behaviors that depend on their accretion rates and the changes in this rate. The highest accretion rates are evident during the bright states of novalikes, as well as the superoutbursts of the shortest p…

2020 Advances in Space Research
eHST 3
NLTE spectral analysis of the intermediate helium-rich subdwarf B star CPD-20°1123
DOI: 10.1093/mnras/staa1686 Bibcode: 2020MNRAS.497...67L

Löbling, L.

Subdwarf B (sdB) stars are core helium-burning stars with stratified atmospheres. Their atmospheres are dominated by hydrogen (H) while the helium (He) and metal abundances are shaped by an interplay of gravitational settling and radiative levitation. However, a small fraction of these show spectra dominated by He I absorption lines. In between th…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 3
Cross-correlating Planck with VST ATLAS LRGs: a new test for the ISW effect in the Southern hemisphere
DOI: 10.1093/mnras/staa592 Bibcode: 2020MNRAS.493.4830A

Metcalfe, Nigel; Shanks, Tom; Ansarinejad, Behzad +1 more

The integrated Sachs-Wolfe (ISW) effect probes the late-time expansion history of the Universe, offering direct constraints on dark energy. Here, we present our measurements of the ISW signal at redshifts of $\bar{z}=0.35$ , 0.55, and 0.68, using the cross-correlation of the Planck cosmic microwave background temperature map with ∼0.5 million lumi…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 3
Observation of Disturbed Plasma Structures in the Environment of the Sun and Near-Earth Space with Radio Sounding and Local Measurements
DOI: 10.1134/S0010952520060040 Bibcode: 2020CosRe..58..460E

Bird, M. K.; Efimov, A. I.; Lukanina, L. A. +3 more

An experiment on radio sounding of the circumsolar plasma by signals from the Mars Express spacecraft in 2013 was carried out in the period from March 4 through May 31. The investigated characteristics were the frequency of signals in the centimeter and decimeter ranges and the differential frequency. A number of events were recorded in which the …

2020 Cosmic Research
MEx SOHO 3
New CCD photometry and light curve analysis of two WUMaBinaries: 1SWASP J133417.80+394314.4 and V2790 Orion
DOI: 10.1016/j.newast.2020.101400 Bibcode: 2020NewA...8001400S

El-Depsey, M. H.; Hassan, I. A.; Shokry, A. +5 more

We present a new multicolor CCD photometry and light curve analysis of two eclipsing binary systems, 1SWASP J133417.80 + 394314.4 and V2790 Orion. The photometric solutions for both binaries were carried out using the updated version of the Wilson- Devinney code. The results showed that first systems is A- type W UMa with mass ratios q = 0.158 whi…

2020 New Astronomy
Gaia 3
Accuracy of magnitudes in pre‑telescopic star catalogs
DOI: 10.1002/asna.202013803 Bibcode: 2020AN....341..827P

Hoffmann, Susanne M.; Protte, Philipp

Historical star magnitudes from catalogs by Ptolemy (137 AD), al‑Sūfī (964), and Tycho Brahe (1602/27) are converted to the Johnson V‑mag scale and compared to modern‑day values from the HIPPARCOS catalog. The deviations (or "errors") are tested for dependencies on three different observational influences. The relation between historical and moder…

2020 Astronomische Nachrichten
Hipparcos 3
The Composition, Excitation, and Physical State of Atomic Gas in the Debris Disk Surrounding 51 Oph
DOI: 10.3847/1538-4357/ab8bdd Bibcode: 2020ApJ...896...24J

Jenkins, Edward B.; Gry, Cécile

We measured 304 absorption features in the ultraviolet and visible spectra of the star 51 Oph, which is known to have a debris disk with a high inclination. We analyzed the relative populations of atoms in excited fine-structure and metastable levels that are maintained by optical pumping and collisional excitation by electrons, and we found that …

2020 The Astrophysical Journal
eHST 3
The fractal nature as new frontier in microstructural characterization and relativization of scale sizes within space
DOI: 10.1142/S0217984920504217 Bibcode: 2020MPLB...3450421M

Arnold, Walter; Mitic, Vojislav V.; Lazovic, Goran +3 more

Today in the age of advanced ceramic civilization, there are a variety of applications for modern ceramics materials with specific properties. Our up-to date research recognizes that ceramics have a fractal configuration nature on the basis of different phenomena. The key property of fractals is their scale-independence. The practical value is tha…

2020 Modern Physics Letters B
Rosetta 3
The fate of O+ ions observed in the plasma mantle: particle tracing modelling and cluster observations
DOI: 10.5194/angeo-38-645-2020 Bibcode: 2020AnGeo..38..645S

Nilsson, Hans; Gunell, Herbert; Slapak, Rikard +5 more

Ion escape is of particular interest for studying the evolution of the atmosphere on geological timescales. Previously, using Cluster-CODIF data, we investigated the oxygen ion outflow from the plasma mantle for different solar wind conditions and geomagnetic activity. We found significant correlations between solar wind parameters, geomagnetic ac…

2020 Annales Geophysicae
Cluster 3
Two New Rapidly Rotating ON Stars Found with LAMOST
DOI: 10.3847/1538-4357/ab5b01 Bibcode: 2020ApJ...888...81L

Howarth, Ian D.; Li, Guang-Wei

The ON stars are a rare subtype of O stars of uncertain origin. We report two new, rapidly rotating ON stars found in data acquired with the Large Sky Area Multi-Object Fiber Spectroscopic Telescope. LS I +61 28 is an ON8.5 Vn dwarf with a projected equatorial rotational velocity of {V}{{e}}\sin I≃ 298 {km} {{{s}}}-1, while H…

2020 The Astrophysical Journal
Gaia 3