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The oxygen abundances for four dwarf spiral galaxies have been determined using long-slit spectroscopy. The abundances of these galaxies have not previously reported in the literature. Several HII reg...
The oxygen gradient of four dS galaxies has been determined using abundances for several Hii regions determined with four different methods. The gradient slopes of the three non-barred galaxies in t...
Measurements made with the Ultraviolet Coronagraph Spectrometer (UVCS) on the Solar and Heliospheric Observatory can be used to determine physical parameters in the solar corona such as hydrogen and i...
New spectroscopic observations of dwarf nova BZ ursae Majoris with extremely unusual emission lines profiles
Fe II in the orion nebula:spectroscopic observations and theoretical models。
Measurements made with the Ultraviolet Coronagraph Spectrometer (UVCS) on the Solar and Heliospheric Observatory can be used to determine physical parameters in the solar corona such as hydrogen a...

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