activity
20172020
most citedNeon Abundances of B-stars in the Solar Neighborhood

14 citations · 24 across the 3 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

5 papers · 1 filter

astro-ph.SR202014 cited

Neon Abundances of B-stars in the Solar Neighborhood

Sofya Alexeeva, Tianxiang Chen, Tatyana Ryabchikova +4

We constructed a comprehensive model atom for NeI -- NeII using the most up-to-date atomic data available and evaluated the non-local thermodynamic equilibrium (NLTE) line formatio…

astro-ph.SR2019

The NLTE Analyses of Carbon Emission Lines in the Atmospheres of O and B type Stars

Sofya Alexeeva, Kozo Sadakane, Masayoshi Nishimura +2

We present a model atom for C I - C II - C III - C IV using the most up-to-date atomic data and evaluated the non-local thermodynamic equilibrium (NLTE) line formation in classical…

astro-ph.SR20193 cited

A Spectroscopic Study of Weak Metallic Emission Lines in a B3V Star iota Her

Kozo Sadakane, Masayoshi Nishimura

We present a list of weak emission lines (WELs) observed in a sharp-lined B3 V star ι Her (HD 160762) using high resolution (R = 65000) and high SN (~1300) spectral data. The list…

astro-ph.SR2018

Spectroscopic abundance analyses of the 3He stars HD 185330 and 3 Cen A

Kozo Sadakane, Masayoshi Nishimura

Abundances of 21 elements in two 3He stars HD 185330 and 3 Cen A have been analysed relative to the well studied sharp-lined B3 V star iota Her. Six elements (P, Ti, Mn, Fe, Ni, an…

astro-ph.SR20177 cited

Weak Metallic Emission Lines in Early B-Type Stars

Kozo Sadakane, Masayoshi Nishimura

Previously unrecognized weak emission lines originating from high excitation states of Si II (12.84 eV) and Al II (13.08 eV) are detected in the red region spectra of slowly rotati…