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    顯示項目326-350 / 370. (共15頁)
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    日期題名作者
    2000 New discovery of weak-line T Tauri stars in high-Galactic latitude molecular clouds Li,JZ; Hu,JY; Chen,WP
    2000 On three-dimensional spiral galaxies Luo,XL; Peng,QH; Long,M; Peng,F; Zou,ZG
    2000 Rotating halos and spirals in low surface brightness galaxies Chiueh,T; Tseng,YH
    2000 Spatially resolved spectrophotometry of M81: Age, metallicity, and reddening maps Kong X; Zhou X; Chen JS; Cheng FZ; Jiang ZJ; Zhu J; Zheng ZY; Mao S; Shang ZH; Fan XH; Byun YI; Chen R; Chen WP; Deng LC; Hester JJ; Li Y; Lin WP; Su HJ; Sun WH; Tsay WS; Windhorst RA; Wu H; Xia XY; Xu W; Xue SJ; Yang HJ; Zheng
    2000 Spectral energy distribution and abundances of NGC 288 stars Chen,ABC; Tsay,WS; Tsai,WS; Lu,PK
    2000 Thermal plasma composition in Saturn's magnetosphere Ip,WH
    2000 Velocity-anisotropy-driven bending instability in the galactic stellar disk Chiueh,T; Wu,JM; Tseng,YH
    1999 Deep intermediate-band surface photometry of NGC 907 Zheng,ZY; Shang,ZH; Su,HJ; Burstein,D; Chen,JS; Deng,ZG; Byun,YI; Chen,R; Chen,WP; Deng,LC; Fan,XH; Fang,LZ; Hester,JJ; Jiang,ZJ; Li,Y; Lin,WP; Sun,WH; Tsay,WS; Windhorst,RA; Wu,H; Xia,XY; Xu,W; Xue,SJ; Yan,HJ; Zheng,Z; Zhou,X; Z
    1999 Discovery of WTTS candidates in high-galactic latitude translucent molecular clouds Li,JZ; Hu,JY; Chen,WP
    1999 Galileo imaging of atmospheric emissions from Io Geissler,PE; McEwen,AS; Ip,W; Belton,MJS; Johnson,TV; Smyth,WH; Ingersoll,AP
    1999 Mid-infrared images of luminous infrared galaxies in a merging sequence Hwang,CY; Lo,KY; Gao,Y; Gruendl,RA; Lu,NY
    1999 Quiescent prominence equilibria Chiueh,T; Lin,LCC
    1999 Radiation field in a superstrong magnetoactive electron plasma Chou,CK
    1998 A comparison of different cluster mass estimates: Consistency or discrepancy? Wu,XP; Chiueh,T; Fang,LZ; Xue,YJ
    1998 A critical analysis of ideal magnetohydrodynamic models for crab-like pulsar winds Chiueh,T; Li,ZY; Begelman,MC
    1998 Ambipolar diffusion-driven tearing instability in a steepening background magnetic field Chiueh,T
    1998 Ring structure and warp of NGC 5907: Interaction with dwarf galaxies Shang,ZH; Zheng,ZY; Brinks,E; Chen,JS; Burstein,D; Su,HJ; Byun,YI; Deng,LC; Deng,ZG; Fan,XH; Jiang,ZJ; Li,Y; Lin,WP; Ma,F; Sun,WH; Wills,B; Windhorst,RA; Wu,H; Xia,XY; Xu,W; Xue,SJ; Yan,HJ; Zhou,X; Zhu,J; Zou,ZL
    1998 Scale invariance of rich cluster abundance: A possible test for models of structure formation Xu,W; Fang,LZ; Wu,XP
    1998 Steps toward determination of the size and structure of the broad-line region in active galactic nuclei. XIII. Ultraviolet observations of the broad-line radio galaxy 3C 390.3 O'Brien,PT; Dietrich,M; Leighly,K; Alloin,D; Clavel,J; Crenshaw,DM; Horne,K; Kriss,GA; Krolik,JH; Malkan,MA; Netzer,H; Peterson,BM; Reichert,GA; Rodriguez-Pascual,PM; Wamsteker,W; Anderson,KSJ; Bochkarev,NG; Cheng,FZ; Filippenko,AV; Gas
    1998 Surface photometry of edge-on galaxies: IC 5249 and ESO 404-G18 Byun,YI
    1997 Charged magnetosonic solitons propagating in gentle density gradients and wave breaking Chiueh,T; Juang,FR
    1997 Cosmic-ray-modified shocks with injection in the hydrodynamic approach .1. Injection linear in the thermal pressure Ko,CM; Chan,KW; Webb,GM
    1997 Radiation pressure in a superdense electron plasma Chou,CK
    1997 Steps toward determination of the size and structure of the broad-line region in active galactic nuclei .11. Intensive monitoring of the ultraviolet spectrum of NGC 7469 Wanders,I; Peterson,BM; Alloin,D; Ayres,TR; Clavel,J; Crenshaw,DM; Horne,K; Kriss,GA; Krolik,JH; Malkan,MA; Netzer,H; OBrien,PT; Reichert,GA; RodriguezPascual,PM; Wamsteker,W; Alexander,T; Anderson,KSJ; Benitez,E; Bochkarev,NG; Burenkov
    1997 The distance to the Hyades cluster based on Hubble Space Telescope Fine Guidance Sensor parallaxes vanAltena,WF; Lu,CL; Lee,JT; Girard,TM; Guo,X; Deliyannis,CP; Platais,I; KozhurinaPlatais,V; McArthur,B; Benedict,GF; Duncombe,RL; Hemenway,PD; Jefferys,WH; King,JR; Nelan,E; Shelus,PS; Story,D; Whipple,A; Franz,OG; Wasserman,L; Freder

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