Nahar, Sultana N.
সুলতানা নুরুন নাহার
Nahar, Sultana Nurun
Nahar, Sultana (Sultana N.), astronoom
VIAF ID: 158515283 (Personal)
Permalink: http://viaf.org/viaf/158515283
Preferred Forms
- 200 _ | ‡a Nahar ‡b Sultana N.
- 100 1 _ ‡a Nahar, Sultana N.
- 100 1 _ ‡a Nahar, Sultana N.
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- 100 1 _ ‡a Nahar, Sultana Nurun
- 100 1 _ ‡a Nahar, Sultana Nurun
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- 100 0 _ ‡a সুলতানা নুরুন নাহার
4xx's: Alternate Name Forms (14)
Works
Title | Sources |
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Absolute photoionization cross section measurements of O II ions from 29.7 to 46.2 eV | |
Atomic astrophysics and spectroscopy | |
Atomic data from the iron project. LXI. Radiative E1, E2, E3, and M1 transition probabilities for Fe IV | |
Broadband, monochromatic and quasi-monochromatic x-ray propagation in multi-Z media for imaging and diagnostics | |
A collection of model stellar spectra for spectral types B to early-M | |
Collision strengths for FIR and UV transitions in P III and the phosphorus abundance | |
A higher-than-predicted measurement of iron opacity at solar interior temperatures | |
Improved collision strengths and line ratios for forbidden [O III] far-infrared and optical lines | |
The iron project and the RmaX project: analysis of Optical/NIR and X-ray spectra of iron from active galactic nuclei | |
Large Enhancement in High-Energy Photoionization of Fe XVII and Missing Continuum Plasma Opacity. | |
Nahar and Pradhan Reply | |
[Oii] line ratios | |
On the importance of satellite lines to the helium-like K{alpha} complex and the G ratio for calcium, iron and nickel | |
Photoionization and electron-ion recombination of P II | |
Photoionization of ground and excited states of Ti I | |
Relativistic fine structure oscillator strengths for Li-like ions: C IV - Si XII, S XIV, Ar XVI, Ca XVIII, Ti XX, Cr XXII, and Ni XXVI | |
Theoretical Fe I-III emission-line strengths from active galactic nuclei with broad-line regions | |
Tumoricidal activity of low-energy 160-KV versus 6-MV X-rays against platinum-sensitized F98 glioma cells | |
Unified electronic recombination of Ne-like Fe XVII: implications for modeling X-ray plasmas | |
X-ray absorption via K{alpha} resonance complexes in oxygen ions |