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Estimating Black Hole Masses of AGNs using Ultraviolet Emission Line Properties
DOI: 10.1088/1009-9271/6/4/02 Bibcode: 2006ChJAA...6..396K

Wang, Ran; Wu, Xue-Bing; Kong, Min-Zhi +1 more

Based on measured broad line region sizes in the reverberation-mapping AGN sample, two new empirical relations are introduced to estimate the central black hole masses of radio-loud high-redshift (z>0.5) AGNs. First, using the archival IUE/HST spectroscopy data at UV band for the reverberation-mapping objects, we obtained two new empirical rela…

2006 Chinese Journal of Astronomy and Astrophysics
IUE 46
Nuclear Starburst Activity in the Seyfert 2 Galaxy NGC 2273
DOI: 10.1088/1009-9271/3/3/203 Bibcode: 2003ChJAA...3..203G

Gu, Qiu-Sheng; Lei, Shi-Jun; Shi, Lei +2 more

We present spectrophotometric results of the Seyfert 2 galaxy NGC 2273. The presence of high-order Balmer absorption lines (H8, H9, H10) and weak equivalent widths of CaII K λ3933, CN λ4200, G-band λ4300 and MgIb λ5173 clearly indicate recent star-forming activity in the nuclear region. Using a simple stellar population synthesis model, we find th…

2003 Chinese Journal of Astronomy and Astrophysics
IUE 5
Measuring the Fundamental Parameters of Hot Hydrogen-Rich White Dwarfs
DOI: 10.1088/1009-9271/3/4/287 Bibcode: 2003ChJAA...3..287B

Barstow, M. A.

This review considers the observations of hot, hydrogen-rich white dwarf stars, with particular reference to measurements of temperature, surface gravity and composition. Spectroscopic data from a variety of wavelength ranges are required for this work and, in particular, the important contributions from optical, ultraviolet and extreme ultraviole…

2003 Chinese Journal of Astronomy and Astrophysics
IUE 0
Infall and Outflow Activities in the Be star FY CMa
DOI: 10.1088/1009-9271/1/6/514 Bibcode: 2001ChJAA...1..514C

Cao, Hui-Lai

Unusual activity of outflow mass motion connected with infall events was recorded for the B0.5 IVe star FY CMa in February 1987 from both archival IUE spectrograms of circumstellar N resonance lines and optical spectra of Hα and He λ5876 Å emission lines which showed inverse P Cygni-type profiles. We estimate the mass loss rate using ultraviolet S…

2001 Chinese Journal of Astronomy and Astrophysics
IUE 3