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Ontology type: schema:Periodical     


Journal Info

START YEAR

N/A

PUBLISHER

Springer US

LANGUAGE

en

HOMEPAGE

http://link.springer.com/journal/10511

Recent publications latest 20 shown

  • 2019-03-01 H-Functions in Radiative Transfer Theory: Calculation of Voigt Functions and Justification of a Model for Formation of Cyclotron Lines in the Spectra of Neutron Stars
  • 2019-03-01 The Effect of Neutrino Mass in Cosmology
  • 2019-02-28 Relationship Between the Ionization Energy and the Radial Velocity of the Ionized Gas in Gaseous Nebulae
  • 2019-02-28 Variable Circumstellar Extinction in UX Ori Stars of Late Spectral Types: V695 Per
  • 2019-02-28 Short-Term Spectral Variability of the Herbig Ae/Be Star HD37806
  • 2019-02-28 Surface Photometry of Dwarf Irregular Galaxies in Different Environments
  • 2019-02-28 Brightness Variability of 12 ROTD A-Stars
  • 2019-02-28 Galaxies with Polar Structures at z > 0.1
  • 2019-02-28 Diffuse Interstellar Bands as Absorption by Frozen Oriented Gas
  • 2019-02-28 HH 276, A Collimated Flux in the Region of FS Tau A/B
  • 2019-02-28 Measurement of the Polytropic Index During Solar Coronal Rain Using a Diagram of the Electron Density Distribution as a Function of Electron Temperature
  • 2019-02-28 Groups and their Representations in the Theory of Radiative Transfer. III.
  • 2018-12 Dynamic Cosmological Tests
  • 2018-12 Magnetic Field of Neutron Stars with a Quark Core
  • 2018-12 Hybrid Stars in the Framework of the Local Nambu-Jona-Lasinio Model for Quark Matter
  • 2018-12 Equation of State for Hot Quark Matter with Neutrino Confinement
  • 2018-12 Study of Brightness Variability of the Components of the Visual Binary System 61 Cyg Based on Observations at the Normal Astrograph of the Pulkovo Observatory
  • 2018-12 On the Possibility of Particle Acceleration in Shock Waves in WR Nebulae
  • 2018-12 BVRI Photometric Observations and Study of the Newly Discovered W UMa Type Eclipsing Binary of Multiple System 1SWASP J093010.78+533859.5
  • 2018-12 Progress in Studies of the Evolution of the Magnetic Fields of CP-Stars. II.
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