The Relation Between BL Loc Objects and OVV Quasars;

BL　Lac天體與OVV類星體的關系

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;

基于自適應徑向基神經網(wǎng)絡的類星體光譜自動識別方法

A Method for Redshift Determination of Quasars Based on CrossCorrelation;

一種基于交叉相關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被證認為一個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.

從大量文獻資料中，收集了類星體3C345光學B波段的有效觀測數(shù)據(jù)點共1642個，獲得了從1896年至1993年的歷史光變曲線。