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We discuss needs in dielectronic recombination data motivated by recent work directed at a quantitative understanding of ion charge states of various elements observed in situ in the solar wind and CM...
We apply the ring diagram technique to source regions of halo coronal mass ejections (CMEs) to study changes in acoustic mode parameters before, during, and after the onset of CMEs.We find that CME re...
Photometric observations of the over-contact binary ER ORI were performed during November 2007 and February to April 2008 with the 51 cm telescope of Biruni Observatory of Shiraz University in U, B an...
Naturally Enhanced Ion Acoustic Lines (NEIALs) detected with Incoherent Scatter Radars (ISRs) can be produced by a Langmuir decay mechanism, triggered by a bump on tail instability. A recent model ...
Venus and Earth have long been thought of as sister planets. Given its similar size and proximity to Earth in the inner Solar System, Venus might seem like a promising candidate for having a surface t...
We conduct a comprehensive analysis of the relationship between central galaxies and their host dark matter halos, as characterized by the stellar mass-halo mass (SM-HM) relation, with rigorous consid...
Anyone who has watched videos of the Apollo astronauts moving across the surface of the moon has noticed the unusual loping gait they sometimes adopted and their slow, almost graceful, movements. Now ...
Analysis of chromatic effects in the shift-and-add method。
Spectral Classification and Analysis of Nuclear Activity in the UZC-Compact Group Sample。
Statistical analysis of molecular line emission from T tauri disk models
Orbit, masses and spectral analysis of the visual binary a 2329。
A 1.4 GHZ and 14.7 GHZ analysis of density gradients in galactic planetary nebulae。
Galactic Planetary Nebulae with Wolf-Rayet Nuclei III. Kinematical Analysis of a Large Sample of Nebulae。
Analysis of Hubble Space Telescope Fine Guidance Sensor Data in TRANS Mode:An Overview。
Quantitative Spectral Classification. Analysis of K-M Giant Stars in the Visible and Near-IR region。

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