Search Publications

Spectrum of imbalanced Alfvénic turbulence at ion-kinetic scales in the solar wind
DOI: 10.1007/s10509-020-03865-8 Bibcode: 2020Ap&SS.365..149G

Voitenko, Y. M.; Gogoberidze, G.

Using a semi-phenomenological model of the imbalanced Alfvénic turbulence, we study the turbulence transition from magnetohydrodynamic to sub-ion kinetic scales in the conditions typical for the fast solar wind. We show that the transition takes place in a wide wave number interval where the energy spectrum does not follow any power law. For large…

2020 Astrophysics and Space Science
Cluster 1
HD 54361: evidence for the status of a low mass TP-AGB star
DOI: 10.1007/s10509-020-3739-1 Bibcode: 2020Ap&SS.365...27Z

Schmidt, M.; Sperauskas, J.; Začs, L. +3 more

The mass of the cool carbon star HD 54361 was suspected to be high, assuming the membership in the stellar association CMa OB1, in conflict with the theory of stellar evolution. The Gaia parallax and a high-resolution spectrum in the wavelength region from about 4800 to 6900 Å was employed in order to update the distance, atmospheric parameters an…

2020 Astrophysics and Space Science
Gaia 0
Exoplanet system Kepler-2 with comparisons to Kepler-1 and 13
DOI: 10.1007/s10509-020-03789-3 Bibcode: 2020Ap&SS.365...77R

Budding, Edwin; Rhodes, Michael D.; Banks, Timothy S. +1 more

We have carried out an intensive study of photometric (Kepler Mission) and spectroscopic data on the system Kepler-2 (HAT-P-7A) using the dedicated software WINFITTER 6.4. The mean individual data-point error of the normalized flux values for this system is 0.00015, leading to the model's specification for the mean reference flux to an accuracy of…

2020 Astrophysics and Space Science
Gaia 0
Measuring the Hubble constant and spatial curvature from supernova apparent magnitude, baryon acoustic oscillation, and Hubble parameter data
DOI: 10.1007/s10509-019-3627-8 Bibcode: 2019Ap&SS.364..134P

Park, Chan-Gyung; Ratra, Bharat

Cosmic microwave background (CMB) anisotropy (spatial inhomogeneity) data provide the tightest constraints on the Hubble constant, matter density, spatial curvature, and dark energy dynamics. Other data, sensitive to the evolution of only the spatially homogeneous part of the cosmological model, such as Type Ia supernova apparent magnitude, baryon…

2019 Astrophysics and Space Science
eHST 86
Observational constraints on the tilted flat-XCDM and the untilted nonflat XCDM dynamical dark energy inflation parameterizations
DOI: 10.1007/s10509-019-3567-3 Bibcode: 2019Ap&SS.364...82P

Park, Chan-Gyung; Ratra, Bharat

We constrain tilted spatially-flat and untilted nonflat XCDM dynamical dark energy inflation parameterizations using Planck 2015 cosmic microwave background (CMB) anisotropy data and recent baryonic acoustic oscillations distance measurements, Type Ia supernovae data, Hubble parameter observations, and growth rate measurements. Inclusion of the fo…

2019 Astrophysics and Space Science
eHST 86
CCD UBV photometric and Gaia astrometric study of eight open clusters—ASCC 115, Collinder 421, NGC 6793, NGC 7031, NGC 7039, NGC 7086, Roslund 1 and Stock 21
DOI: 10.1007/s10509-019-3640-y Bibcode: 2019Ap&SS.364..152Y

Paunzen, E.; Güver, T.; Bilir, S. +8 more

In this study, we carried out CCD UBV photometry of eight open clusters, ASCC 115, Collinder 421, NGC 6793, NGC 7031, NGC 7039, NGC 7086, Roslund 1, Stock 21, and determined their reddening, metallicity, distance, age, and mass functions. We used new Gaia Data Release 2 (DR2) astrometric data to separate cluster member stars from the field stars a…

2019 Astrophysics and Space Science
Gaia 21
Radio emission from interstellar shocks: Young type Ia supernova remnants and the case of N 103B in the Large Magellanic Cloud
DOI: 10.1007/s10509-019-3696-8 Bibcode: 2019Ap&SS.364..204A

Haberl, F.; Filipović, M. D.; Rowell, G. +19 more

We investigate young type Ia supernova remnants (SNRs) in our Galaxy and neighbouring galaxies in order to understand their properties and early stage of their evolution. Here we present a radio continuum study based on new and archival data from the Australia Telescope Compact Array (ATCA) towards N 103B, a young (≤1000 yrs) spectroscopically con…

2019 Astrophysics and Space Science
eHST 14
A young multipolar planetary nebula in the making—IRAS 21282+5050
DOI: 10.1007/s10509-019-3523-2 Bibcode: 2019Ap&SS.364...32H

Zhang, Yong; Kwok, Sun; Hsia, Chih-Hao +1 more

We present high-angular-resolution Hubble Space Telescope (HST) optical and near-infrared imaging of the compact planetary nebula (PN) IRAS 21282+5050. Optical images of this object reveal several complex morphological structures including three pairs of bipolar lobes and an elliptical shell lying close to the plane of the sky. From near-infrared …

2019 Astrophysics and Space Science
AKARI Gaia ISO eHST 10
Implication of kinetic Alfvén waves to magnetic field turbulence spectra: Earth's magnetosheath
DOI: 10.1007/s10509-019-3592-2 Bibcode: 2019Ap&SS.364..101D

Khodachenko, M. L.; Kumar, S.; Echim, M. +5 more

In the present paper, we investigate the power-law behaviour of the magnetic field spectra in the Earth's magnetosheath region using Cluster spacecraft data under solar minimum condition. The power spectral density of the magnetic field data and spectral slopes at various frequencies are analysed. Propagation angle,

2019 Astrophysics and Space Science
Cluster 9
The analysis of effective galaxies number count for Chinese Space Station Optical Survey (CSS-OS) by image simulation
DOI: 10.1007/s10509-019-3501-8 Bibcode: 2019Ap&SS.364....9Z

Zhang, Xin; Meng, Xianmin; Cao, Li

The Chinese Space Station Optical Survey (CSS-OS) is a mission to explore the vast universe. This mission will equip a 2-meter space telescope to perform a multi-band NUV-optical large area survey (over 40% of the sky) and deep survey (

2019 Astrophysics and Space Science
eHST 8