The Relation Between BL Loc Objects and OVV Quasars;
BL Lac天體與OVV類星體的關(guān)系
Evolution of Lyα Forest in High-resolution Spectroscopy of QSOs;
類星體高分辨率光譜中Lyα森林的演化
The Relation between the Cerenkov Line Radiation of Superlight Electron and the Emission-Line Spectra of QSOs;
類星體輻射與契倫科夫射線關(guān)系的探討
The Periodicity in Redshift Distribution of QSOs;
類星體紅移分布的周期性
Automated Recognition of Quasars Based on Adaptive Radial Basis Function Neural Networks;
基于自適應(yīng)徑向基神經(jīng)網(wǎng)絡(luò)的類星體光譜自動(dòng)識(shí)別方法
A Method for Redshift Determination of Quasars Based on CrossCorrelation;
一種基于交叉相關(guān)的類星體的紅移測量方法
The physics of broad absorption line quasars;
寬吸收線類星體物理研究
Grand unified theory,lepton stars andgamma-ray bursts,quasars;
大統(tǒng)一理論,輕子星和γ射線暴,類星體(英文)
Two Equally Effective Explanations for the Energy-Liberating Mechanism of Quasars;
類星體放能機(jī)制的兩種等效解釋
TITLE:A NEW DISCOVERED QSO WITH REDSHIFT 1.66;
新發(fā)現(xiàn)的一顆Z＝1．66類星體
ROSAT X-ray Source 1057+4316 Identified as a QSO of z=0.32Z;
ROSAT X射線源1057＋4316被證認(rèn)為一個(gè)z＝0．32的類星體
Absorption Line Spectrum of QSO 1331+170;
類星體1331+170的吸收線光譜
All the data for the B band of the quasar 3C345, presented in twenty-one publications and dating back to 1896, have been compiled to be a light curve.
從大量文獻(xiàn)資料中，收集了類星體3C345光學(xué)B波段的有效觀測數(shù)據(jù)點(diǎn)共1642個(gè)，獲得了從1896年至1993年的歷史光變曲線。