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Journals   A B C D E F G H I J K L M N O P Q R S T U V W X Y Z
Zijinshan Tianwentai Taikan
1000-3681
1999 Issue 3
MULTI WAVELENGTH QUASAR SURVEY
he xiang tao wu jiang hua (department of astronomy; beijing normal university; beijing 100875)
..............page:3-8
RADIO IMAGES OF EGRET DETECTED AGN
hong xiao yu jiang dong rong (shanghai observatory; academia sinica; shanghai; 200030) (national astronomical obserratories; chinese academ of sciences; beijing; 100012)
..............page:31-34
DUST EFFECT IN GAMMA RAY LOUD BLAZARS
xie guang zhong 1; 2; 3; 4 mei dong chang 1; 2; 3 bai jin ming 1; 2; 3 (yunnan astronomical observatory; chinese academy of science; p.o.box 110; kunming; 650011; china(gzxie@public.km.yn.cn) 1; (national astronomical observatories; chinese
..............page:9-21
LINK BETWEEN DISKS AND JETS IN RADIO LOUD ACTIVE GALACTIC NUCLEI
cao xin wu 1; 2 jiang dong rong 1; 2 ( shanghai astronomical observatory; academia sinica; shanghai; 200030) 1 ( national astronomical observatories; chinese academy of sciences; beijing; 100012; email: cxw@center.shao.ac.cn) 2
..............page:35-39
RECENT PROGRESS ON THE BAL QSOS RESEARCH FROM X RAY OBSERVATIONS
wang ting gui wang jun xian (center for astrophysics; university of science and technology; hefei; 230026)
..............page:40-45
THE VARIABILITY OF OPTICALLY SELECTED QSO SAMPLE
huang ke liang zhou hong nan (physics department; nanjing normal university; nanjing 210097; prc)
..............page:22-26
DIAGNOSIS OF AMBIENT PARAMETERS IN A SOURCE OF MICROWAVE SPIKES ON NOV.2,1997
huang guang li (purple mountain observatory; academia sinica; nanjing 210008)
..............page:135-141
AN HST SURFACE PHOTOMETRIC STUDY OF ULTRALUMINOUS INFRARED GALAXIES
zheng zhen 1 wu hong 1 mao shu de 2 xia xiao yang 3 deng zhu gan 4 zhou zhen long 1 (beijing astronomical observatory; chinese academy of sciences.beijing; 100012) 1 (max planck institute for astrophysics; germany) 2 (department of
..............page:49-51
SEVERAL PROBLEMS ON TYPE Ia SUPERNOVAE
li zong wei 1 wang xiao feng 1 pei shou yong 2 (department of astronomy; beijing normal university; beijing 100875) 1 (department of physics; beijing normal university; beijing 100875) 2 email to: lizw@bnu.edu.cn
..............page:95-102
SMALL AMPLITUDE HORIZONTAL BRANCH VARIABLE STARS NEAR THE RED BOUNDARY OF THE INSTABILITY STRIP IN M3
yao bao an 1 shen chang jun 2 zhang chun sheng 2 qing dao 2 (shanghai observatory; academia; shanghai 200030) 1 (purple mountain observatory; academia sinica; nanjing 210008) 2
..............page:113-116
NUMERICAL SIMULATION OF THE MAGNETIC RECONNECTION IN SOLAR FLARES
fang cheng chen peng fei di xiao hua ding ming de tang yu hua (department of astronomy; nanjing university; nanjing 210093)
..............page:122-125
ELECTRON POSITRON ANNIHILATION LINE IN SOLAR FLARES
gan wei qun (purple mountain observatory; academia sinica; nanjing; 210008)
..............page:126-129
A STUDY ON VLBI CORE IN AGNS
jiang dong rong zhou jian feng (shanghai observatory; academia sinica; shanghai; 200030) zhou jianfeng (cnao; chinese academia of sciences; beijing; 100012)
..............page:27-30
SPECTROSCOPIC STUDIES OF NOVA CAS 1995
hang heng rong zhu zheng xi liu qing zhong (purple mountain observatory; academia sinica; nanjing 210008) (joint laboratory for optical astronomy; chinese academy of sciences; bejing 100012)
..............page:108-112
THE INFLUENCE OF MAGNETIC FIELD FOR THE RADIATION AND THE STRUCTURE OF NEUTRON STARS
zhang jia l (center for astrophysics; university of science and technology; hefei 230026)
..............page:71-75
NEW MAGNETIC RECONNECTION THEORY
li xiao qing zhang zhen da (department of physics; nanjing normal university; nanjing 210097) z.d.zhang (department of astronomy; nanjing university; nanjing 210093)
..............page:130-134
A MODIFIED LOCAL MIXING LENGTH THEORY
xiong da run 1; 3 deng li cai 2; 3; 4 (purple mountain observatory; academia sinica; nanjing 210008) 1 (beijing astronomical observatory; chinese academy of sciences; beijing 100012) 2 (national astronomical observatory; chinese academy of
..............page:117-121
THE ROLE OF STAR FORMATION IN LINERS
ji li chen yang huang jie hao gu qiu sheng lei shi jun (department of astronomy; nanjing university; nanjing 210093; china draft version july 23; 1999)
..............page:52-62
SUMMARY ON SOLAR SPECTRAL METHODS AND APPLICATION STUDIES OF “MULTI-CLOUD” MODEL
gu xiao ma li ke jun qu zhong quan zhong shu hua dun jin ping (yunnan observatory; academia sinica; kunming 650011)
..............page:142-146
METAL RICH QUASAR AND ACTIVE GALACTIC NUCLEI HOST γ RAY BURSTS
wang jian min 1; 2 (laboratory of cosmic ray and high energy astrophysics; institute of high energy physcis; cas; beijing 100039) 1 (cas pku joint beijing astrophysical conter; beijing 100871) 2
..............page:63-65
STELLAR POPULATION SYNTHESIS FOR BLUE COMPACT GALAXIES
chen fu zhen 1; 2 kong xu 1; 3 (center for astrophysics; university of science and technology of china; 230026; hefei; p.r.china; email:xkong@mail.ustc.edu.cn) 1 (national astronomical observatories; chinese academy of sciences; 100012; beiji
..............page:66-70
INVERSE COMPTON SCATTERING (ICS) MODEL AND POLARIZATION OBSERVATIONS OF RADIO PULSARS
qiao guo jun xu ren xin han jin lin zhang bing hong bi hai liu ji feng (bac 2 and astronomy department; peking university; beijing 100871; china)
..............page:76-84
THE STUDY OF GEOMETRY ASYMMETRY OF MEAN PULSE PROFILE OF PULSAR
wu xin ji pan jun (department of geophysics; peking university and chinese academy ofscience peking university joint beijing astrophysical center; beijing 100871; p.r.china)
..............page:91-94
X RAY ANALYSES OF SUPERNOVA REMNANTS
chen yang wang zhen ru sun ming bai lei (department of astronomy; nanjing university; nanjing 210093)
..............page:103-107
THE EFFECT OF ICS ON GRB AFTERGLOWS
wei da ming (purple mountain observatory; academia sinica; nanjing 210008 )
..............page:85-90
THE IRON 6.4 Kev K_α OBSERVATIONS AND SUSPICIONS ON THE DISC LINE MODELS
you jun han ( institute for space and astrophysics ; department of applied physics; shanghai jiao tong university; shanghai; 200030)
..............page:46-48