..............page:387-391
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..............page:264-268
..............page:114-119
..............page:373-377
census of kuiper comets-the taos project
wen ping chenother taos team members: c. alcock; k. cook; s. marshall; m. hammergren(llnl); t. lee; c. yuan; c. y. wen; s. k. king(asiaa); w. s. tsay; w. ip; c. lemme; j. h. wang(ncu); t. axelrod(anu); i. de pater(ucb); j.lissauer(ames); y. i. byun(yonsei
..............page:182-189
model of spectral fluxes for solar spectrograph
cao wenda; song qian (yunnan observatory; the chinese academy of sciences; kunming 650011; china) (national astronomical observatories; the chinese academy of sciences; beijing 100012; china)
..............page:401-405
..............page:392-396
bl lac objects and unified model
fan j.h. (yunnan observatory; the chinese academy of sciences; kunming 650011; china) (national astronomical observatories; the chinese academy of sciences) (center for astrophysics; guangzhou normal university; guangzhou 510400; china e mail: jhfan@g
..............page:210-212
the nature of lyman-break galaxies
shu chenggang 1; 2; 3; 4 ; yin xiao 1; 3; 4 1 (shanghai astronomical observatory; the chinese academy of sciences; shanghai 200030; china) 2 (max planck institut f r astrophysik karl schwarzschild strasse 1; 85748 garching; germany) 3 (nationa
..............page:197-204
..............page:130-133
oh/ir stars with carbon-rich envelope
chen p. s.; wang x. h.; he j. h. (yunnan observatory & united laboratory of optical astronomy cas) (national astronomical observatories; cas; china)
..............page:339-343
infrared low-resolution spectra of haebe stars
chen p. s.; wang x. h.; he j. h. (yunnan observatory and united laboratory for optical astronomy; the chinese academy of sciences; kunming 650011; china) (national astronomical observatories; cas; china)
..............page:344-348
..............page:328-332
..............page:363-367
dual channel sis receiver of trao telescope
jong ae park 1; 2 ; seog tae han 1; tai seong kim 1; kwang dong kim 1; hyo ryoung kim 1; hyun soo chung 1; jae hoon jung 1; chang hoon lee 1; se hyung cho 1; jongmann yang 2 1. taeduk radio astronomy observatory (trao); hwaam dong
..............page:82-85
..............page:354-357
..............page:143-146
..............page:147-152
vibi observations of two quasars at 1.3cm
su bumei; li yongsheng ( yunnan observatory; the chinese academy of sciences; kunming 650011; china ) ( national astronomical observatories; the chinese academy of sciences; beijing 100012; china ) braath l.b. ( center for imaging technologies; halmst
..............page:299-304
..............page:124-126
..............page:134-138
near-infrared solar electric field telescope
song guofeng 1 (beijing astronomical observatory; the chinese academy of sciences; beijing 100012; china) 2 (national astronomical observatories; the chinese academy of sciences; beijing 100012; china)
..............page:120-123
..............page:283-287
..............page:103-108
..............page:324-327
..............page:315-318
the near-nuclear study of comet hale bopp
tao jun; qian bochen; gu mingfeng; tang yuan; song baojun (shanghai astronomical observatory; the chinese academy of sciences; shanghai 200030; china) email: taojun@center. shao. ac. cn
..............page:467-470
..............page:428-432
..............page:250-254
..............page:269-273
development of a multi kd~* p controller
y.d.park 1; u.w.nam 1; y. j.moon 1; h.y.kim 2 1 (korea astronomy observatory; taejon 305 348; korea) 2 (department of space science in kyunghee university; seoul 449 701; korea)
..............page:109-113
observations of ultraluminous iras galaxies at 20cm
li yongsheng; su bumei ( yunnan observatory; the chinese academy of sciences; kunming 650011; china ) ( national astronomical observatories; the chinese academy of sciences; beijing 100012; china ) norris r.p. (australia telescope national facility
..............page:305-308
photometric survey of galactic open clusters
m.g. lee 1; h.b. ann 2; m.y. chun 3; s. l. kim 3; y. b. jeon 3; b. g. park 3; i. s. yuk 3; h.sung 4 1 (dept. of astronomy; seoul national university; seoul 151-742; korea; mglee@astrog. snu. ac. kr) 2 (department of earth science; pusan nat
..............page:213-217
..............page:240-244
the chiralities of three filaments in ar7500
jiang yunchun 1; 2; 3 ; luan di 1; 2 ; lin ganghua 1; 3 ; wang jingxiu 1; 3 1 (national astronomical observatories; the chinese academy of sciences; beijing 100012; china) 2 (yunnan observatory; the chinese academy of sciences; kunming 65001
..............page:433-437
..............page:452-456
kiso multi-fiber spectroscope project
yasushi yadoumaru; nobunari itoh; yoshikazu nakada; ken ichi tarusawa; takao soyano kiso observatory; institute of astronomy; the university of tokyo and hiroyuki mito the graduate university for advanced studies
..............page:72-76
..............page:218-221
..............page:222-227
..............page:98-102
..............page:410-413
..............page:419-423
..............page:481-484
..............page:471-475
..............page:260-263
..............page:349-353
..............page:139-142
..............page:319-323
..............page:236-239
..............page:485-487
quasioptical system of trao telescope
jong ae park 1; 2 ; seog tae han 1; tai seong kim 1; kwang dong kim 1; hyo ryoung kim 1; hyun soo chung 1; chang hoon lee 1; se hyung cho 1; jongmann yang 2 1. (taeduk radio astronomy observatory (trao); hwaam dong; yusung gu taejon
..............page:86-89
..............page:205-209
..............page:232-235
..............page:406-409
..............page:397-400
magnetic and velocity fields in flare regions
li wei 1(beijing astronomical observatory; the chinese academy of sciences; beijing 100012; china) 2(national astronomical observatories; the chinese academy of sciences; beijing 100012; china)
..............page:175-181
..............page:457-460
..............page:288-293
..............page:424-427
the study of metallicity indices
nobunari itoh; yasushi yadoumaru; yoshikaze nakada kiso observatory; institute of astronomy; the university of tokyo hiroyuki mito the graduate university for advanced studies
..............page:245-249
hides: a high dispersion echelle spectrograph
hideyuki izumiura okayama astrophysical observatory; national astronomical observatory of japan honjo 3037 5; kamogata; asakuchi; okayama 719 0232; japan e mail: izumiura @ oao. nao. ac. jp
..............page:77-81
..............page:255-259
..............page:294-298
..............page:309-311
..............page:127-129
..............page:414-418
..............page:153-156
..............page:279-282
high x-ray-to-optical flux ratio sources from rass
xu d. w 1; 2 ; wei j. y 1; 2 ; dong x. y 1; 2 ; hu j.y 1; 2 1 (beijing astronomical observatory; the chinese academy of sciences; beijing 100012; china) 2 (national astronomical observatories; the chinese academy of sciences; beijing 10
..............page:312-314
microwave millisecond spikes on july 30, 1997
wang m.; xie r. x.$$$$1 (beijing astronomical observatory; the chinese academy of sciences; beijing 100012; china) 2 (yunnan astronomical observatory; the chinese academy of sciences; kunming 650011; china) 3 (national astronomical observatories; the ch
..............page:461-466
..............page:447-451
..............page:333-338
about the o'connell effect of a close binary
liu qingyao; yang yulan (yunnan observatory; the chinese academy of sciences; kunming 650011; china) (united laboratory of optical astronomy; the chinese academy of sciences; kunming 650011; china) (national astronomical observatories; the chinese acad
..............page:378-382
..............page:383-386
..............page:159-165
..............page:438-441
..............page:442-446
..............page:166-174
..............page:274-278