المؤلفون: Zhang, Chengpeng, Wu, Yuefang, Yuan, Jing-Hua, Liu, Tie

المساهمون: Zhang, CP (reprint author), Peking Univ, Depatment Astron, Beijing 100871, Peoples R China., Peking Univ, Depatment Astron, Beijing 100871, Peoples R China., Chinese Acad Sci, Natl Astron Observatries, Beijing 100012, Peoples R China., Korea Astron & Space Sci Inst, Daejeon 305348, South Korea.

المصدر: SCI

مصطلحات موضوعية: ISM: molecules, ISM: jets and outflows, stars: pre-main-sequence

العلاقة: 315th Symposium of the International-Astronomical-Union.2016,315.; 1534692; http://hdl.handle.net/20.500.11897/460071Test; WOS:000387795900012

الإتاحة: https://doi.org/20.500.11897/460071Test
https://doi.org/10.1017/S1743921316007730Test
https://hdl.handle.net/20.500.11897/460071Test

المؤلفون: Tatematsu, Ken'ichi, Liu, Tie, Ohashi, Satoshi, Sanhueza, Patricio, Quang Nguyen Luong, Hirota, Tomoya, Liu, Sheng-Yuan, Hirano, Naomi, Choi, Minho, Kang, Miju, Thompson, Mark A., Fuller, Gary, Wu, Yuefang, Li, Di, Di Francesco, James, Kim, Kee-Tae, Wang, Ke, Ristorcelli, Isabelle, Juvela, Mika, Shinnaga, Hiroko, Cunningham, Maria, Saito, Masao, Lee, Jeong-Eun, Toth, L. Viktor, He, Jinhua, Sakai, Takeshi, Kim, Jungha

المساهمون: Tatematsu, K (reprint author), Natl Astron Observ Japan, Natl Inst Nat Sci, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan., Tatematsu, K (reprint author), SOKENDAI Grad Univ Adv Studies, Dept Astron Sci, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan., Natl Astron Observ Japan, Natl Inst Nat Sci, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan., SOKENDAI Grad Univ Adv Studies, Dept Astron Sci, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan., Korea Astron & Space Sci Inst, Daedeokdaero 776, Daejeon, South Korea., Univ Tokyo, Dept Astron, Bunkyo Ku, Tokyo 1130033, Japan., Acad Sinica, Inst Astron & Astrophys, 11F Astron Math Bldg,AS NTU 1,Sect 4,Roosvelt Rd, Taipei 10617, Taiwan., Univ Hertfordshire, Sci & Technol Res Inst, Ctr Astrophys Res, Hatfield AL10 9AB, Herts, England., Univ Manchester, Jodrell Bank Ctr Astrophys, Sch Phys & Astron, Oxford Rd, Manchester M13 9PL, Lancs, England., Peking Univ, Dept Astron, Beijing 100871, Peoples R China., Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China., NRC, Herzberg Astron & Astrophys, 5071 West Saanich Rd, Victoria, BC V9E 2E7, Canada., Univ Victoria, Dept Phys & Astron, Victoria, BC V8P IA1, Canada., European Southern Observ, Garching, Germany., Univ Toulouse 3, CNRS, IRAP, UMR5277, 9 Ave Colonel Roche,BP 44346, F-31028 Toulouse 4, France., Univ Helsinki, Dept Phys, FI-00014 Helsinki, Finland., Kagoshima Univ, Dept Phys, 1-21-35 Korimoto, Kagoshima 8900065, Japan., Univ New S Wales, Sch Phys, Sydney, NSW 2052, Australia., Natl Astron Observ Japan, Natl Inst Nat Sci, Nobeyama Radio Observ, Minamisa Ku, Minamimaki, Nagano 3841305, Japan., Kyung Hee Univ, Sch Space Res, Yongin 446701, Gyeonggi Do, South Korea., Eotvos Lorand Univ, Dept Astron, Pazmany Peter Setny 1, H-1117 Budapest, Hungary., Chinese Acad Sci, Yunnan Observ, Key Lab Struct & Evolut Celestial Objects, POB 110, Kunming 650011, Yunnan, Peoples R China., Chinese Acad Sci, South Amer Ctr Astrophys, Camino El Observ 1515, Santiago, Chile., Univ Chile, Dept Astron, Casilla 36-D, Santiago, Chile., Univ Electrocommun, Grad Sch Informat & Engn, Chofu, Tokyo 1828585, Japan.

المصدر: SCI

مصطلحات موضوعية: ISM: clouds, ISM: molecules, ISM: structure, stars: formation, MOLECULAR CLOUD CORES, STAR-FORMING REGIONS, INFRARED DARK CLOUDS, 45-M RADIO TELESCOPE, DENSE CORES, DEUTERIUM FRACTIONATION, CHEMICAL VARIATION, MAPPING OBSERVATIONS, PHYSICAL CONDITIONS, ANGULAR-MOMENTUM

العلاقة: ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES.2017,228(2).; 1909781; http://hdl.handle.net/20.500.11897/475289Test; WOS:000397312100002

الإتاحة: https://doi.org/20.500.11897/475289Test
https://doi.org/10.3847/1538-4365/228/2/12Test
https://hdl.handle.net/20.500.11897/475289Test

المؤلفون: Peng, Yaping, Qin, Sheng-Li, Schilke, Peter, Sanchez-Monge, Alvaro, Wu, Yuefang, Liu, Tie, Li, Di, Moeller, Thomas, Liu, Sheng-Yuan, Feng, Siyi, Liu, Ying, Luo, Gan, Zhang, Li, Rong, Jia-Lei

المساهمون: Peng, YP (reprint author), Yunnan Univ, Dept Astron, Kunming 650091, Peoples R China., Peng, YP (reprint author), Key Lab Astroparticle Phys Yunnan Prov, Kunming 650091, Peoples R China., Yunnan Univ, Dept Astron, Kunming 650091, Peoples R China., Key Lab Astroparticle Phys Yunnan Prov, Kunming 650091, Peoples R China., Univ Cologne, Inst Phys 1, Zulpicher Str 77, D-50937 Cologne, Germany., Peking Univ, Dept Astron, Beijing 100871, Peoples R China., Korea Astron & Space Sci Inst, 776 Daedeokdaero, Daejeon 305348, South Korea., Chinese Acad Sci, Natl Astron Observ, Datun Rd 20A, Beijing, Peoples R China., Acad Sinica, Inst Astron & Astrophys, Taipei, Taiwan., Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany., Hebei Normal Univ, Dept Phys, Shijiazhuang 050024, Peoples R China., Hebei Normal Univ, Hebei Adv Thin Film Lab, Shijiazhuang 050024, Peoples R China.

المصدر: SCI

مصطلحات موضوعية: ISM: abundances, ISM: individual objects (Orion KL), ISM: molecules, radio lines: ISM, stars: formation, C-12/C-13 ISOTOPE RATIO, HOT CORE, MOLECULAR CLOUDS, KINETIC TEMPERATURES, APERTURE SYNTHESIS, MASSIVE STARS, KLEINMANN-LOW, MU-M, MILLIMETER, BN/KL

العلاقة: ASTROPHYSICAL JOURNAL.2017,837(1).; 1909338; http://hdl.handle.net/20.500.11897/474894Test; WOS:000395918600014

الإتاحة: https://doi.org/20.500.11897/474894Test
https://doi.org/10.3847/1538-4357/aa5c81Test
https://hdl.handle.net/20.500.11897/474894Test

المؤلفون: Leurini, S., Herpin, F., van der Tak, F., Wyrowski, F., Herczeg, G. J., van Dishoeck, E. F.

المساهمون: Leurini, S (reprint author), Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany., Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany., INAF Osservatorio Astron Cagliari, Via Sci 5, I-09047 Selargius, CA, Italy., Univ Bordeaux, CNRS, Lab Astrophys Bordeaux, B18N,Allee Geoffroy St-Hilaire, F-33615 Pessac, France., SRON, Netherlands Inst Space Res, POB 800, NL-9700 AV Groningen, Netherlands., Univ Groningen, Kapteyn Astron Inst, NL-9712 Groningen, Netherlands., Peking Univ, Kavli Inst Astron & Astrophys, Yi He Yuan Lu 5, Beijing 100871, Peoples R China., Leiden Univ, Leiden Observ, POB 9513, NL-2300 RA Leiden, Netherlands., Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany.

المصدر: SCI

مصطلحات موضوعية: stars: formation, stars: protostars, ISM: molecules, line: profiles, HOT CORE G327.3-0.6, YOUNG STELLAR OBJECTS, HERSCHEL WISH, PROTOSTELLAR OBJECTS, HIFI OBSERVATIONS, EXCITED-STATES, PROTOSTARS, EVOLUTION, EMISSION, OUTFLOWS

العلاقة: ASTRONOMY & ASTROPHYSICS.2017,602.; 1907115; http://hdl.handle.net/20.500.11897/472930Test; WOS:000404648300104

الإتاحة: https://doi.org/20.500.11897/472930Test
https://doi.org/10.1051/0004-6361/201730387Test
https://hdl.handle.net/20.500.11897/472930Test

المؤلفون: Gama, D. R. G., Lepine, J. R. D., Mendoza, E., Wu, Y., Yuan, J.

المساهمون: Gama, DRG (reprint author), Univ Sao Paulo, Dept Astron, IAG, Sao Paulo, Brazil., Univ Sao Paulo, Dept Astron, IAG, Sao Paulo, Brazil., Peking Univ, Dept Astron, Beijing 100871, Peoples R China., Natl Astron Observ China, Beijing Shi, Peoples R China.

المصدر: SCI

مصطلحات موضوعية: H II regions, ISM: bubbles, ISM: molecules, stars: formation Supporting material: machine-readable table, MILKY-WAY PROJECT, H-II REGIONS, METHANOL MASER EMISSION, YOUNG STELLAR OBJECTS, GALACTIC HII-REGIONS, INTERSTELLAR GRAINS, LINE EMISSION, OUTER GALAXY, SPITZER, ATLASGAL

العلاقة: ASTROPHYSICAL JOURNAL.2016,830(2).; 1517163; http://hdl.handle.net/20.500.11897/458705Test; WOS:000386124600003

الإتاحة: https://doi.org/20.500.11897/458705Test
https://doi.org/10.3847/0004-637X/830/2/57Test
https://hdl.handle.net/20.500.11897/458705Test

المؤلفون: McJunkin, Matthew, France, Kevin, Schindhelm, Eric, Herczeg, Gregory, Schneider, P. Christian, Brown, Alex

المساهمون: McJunkin, M (reprint author), Univ Colorado, Lab Atmospher & Space Phys, 600 UCB, Boulder, CO 80303 USA., Univ Colorado, Lab Atmospher & Space Phys, 600 UCB, Boulder, CO 80303 USA., Southwest Res Inst, 1050 Walnut St,Suite 300, Boulder, CO 80302 USA., Peking Univ, Kavli Inst Astron & Astrophys, Yi He Yuan Lu 5, Beijing 100871, Peoples R China., ESA ESTEC, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands., Univ Colorado, Ctr Astrophys & Space Astron, Boulder, CO 80309 USA.

المصدر: SCI

مصطلحات موضوعية: circumstellar matter, dust, extinction, ISM: molecules, protoplanetary disks, stars: variables: T Tauri, Herbig Ae/Be, ultraviolet: ISM, HUBBLE-SPACE-TELESCOPE, MOLECULAR-HYDROGEN EMISSION, X-RAY-IRRADIATION, LY-ALPHA, INTERSTELLAR EXTINCTION, H-2 EMISSION, YOUNG STARS, ULTRAVIOLET-SPECTRA, ETA-CHAMAELEONTIS

العلاقة: ASTROPHYSICAL JOURNAL.2016,828(2).; 1512602; http://hdl.handle.net/20.500.11897/456927Test; WOS:000384001900004

الإتاحة: https://doi.org/20.500.11897/456927Test
https://doi.org/10.3847/0004-637X/828/2/69Test
https://hdl.handle.net/20.500.11897/456927Test

المؤلفون: Rong, Jialei, Qin, Sheng-Li, Zapata, Luis A., Wu, Yuefang, Liu, Tie, Zhang, Chengpeng, Peng, Yaping, Zhang, Li, Liu, Ying

المساهمون: Rong, JL (reprint author), Yunnan Univ, Dept Astron, Kunming 650091, Peoples R China., Yunnan Univ, Dept Astron, Kunming 650091, Peoples R China., Key Lab Astroparticle Phys Yunnan Prov, Kunming 650091, Peoples R China., Univ Nacl Autonoma Mexico, Ctr Radiostron & Astrofis, Morelia 58089, Michoacan, Mexico., Peking Univ, Dept Astron, Beijing 100871, Peoples R China., Korea Astron & Space Sci Inst, Daejeon 305348, South Korea., Hebei Normal Univ, Dept Phys, Shijiazhuang 050024, Peoples R China., Hebei Normal Univ, Hebei Adv Film Lab, Shijiazhuang 050024, Peoples R China.

المصدر: SCI

مصطلحات موضوعية: stars: formation, ISM: abundances, ISM: individual objects: W51 North, ISM: molecules, radio lines: ISM, MASSIVE STAR-FORMATION, S-BEARING MOLECULES, LINE SURVEY, CHEMICAL DIFFERENTIATION, HOT CORES, ORION-KL, INTERSTELLAR ACETONE, SAGITTARIUS B2(N), FORMING REGIONS, CHEMISTRY

العلاقة: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY.2016,455,(2),1428-1437.; 1398701; http://hdl.handle.net/20.500.11897/438806Test; WOS:000368007100022

الإتاحة: https://doi.org/20.500.11897/438806Test
https://doi.org/10.1093/mnras/stv2406Test
https://hdl.handle.net/20.500.11897/438806Test

المؤلفون: Ge, J. X., He, J. H., Yan, H. R.

المساهمون: Ge, JX (reprint author), Chinese Acad Sci, Yunnan Observ, Key Lab Struct & Evolut Celestial Objects, POB 110, Kunming 650011, Yunnan, Peoples R China., Chinese Acad Sci, Yunnan Observ, Key Lab Struct & Evolut Celestial Objects, Kunming 650011, Yunnan, Peoples R China., Univ Chinese Acad Sci, Beijing 100049, Peoples R China., Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China., DESY, D-15738 Zeuthen, Germany., Univ Potsdam, Inst Phys & Astron, D-14476 Potsdam, Germany., Chinese Acad Sci, Yunnan Observ, Key Lab Struct & Evolut Celestial Objects, POB 110, Kunming 650011, Yunnan, Peoples R China.

المصدر: SCI

مصطلحات موضوعية: astrochemistry, turbulence, ISM: abundances, ISM: clouds, dust, extinction, ISM: molecules, RAY IONIZATION RATE, POLYCYCLIC AROMATIC-HYDROCARBONS, MONTE-CARLO-SIMULATION, MOLECULAR CLOUDS, SURFACE-CHEMISTRY, CHEMICAL-MODELS, MAGNETOHYDRODYNAMIC TURBULENCE, CHARGE FLUCTUATIONS, HYDROGEN MOLECULES, INFRARED-EMISSION

العلاقة: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY.2016,455,(4),3570-3587.; 1398459; http://hdl.handle.net/20.500.11897/438746Test; WOS:000368009300013

الإتاحة: https://doi.org/20.500.11897/438746Test
https://doi.org/10.1093/mnras/stv2560Test
https://hdl.handle.net/20.500.11897/438746Test

المؤلفون: Yuan, Jinghua, Wu, Yuefang, Liu, Tie, Zhang, Tianwei, Li, Jin Zeng, Liu, Hong-Li, Meng, Fanyi, Chen, Ping, Hu, Runjie, Wang, Ke

المساهمون: Wu, YF (reprint author), Peking Univ, Dept Astron, Beijing 100871, Peoples R China., Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing 100012, Peoples R China., Peking Univ, Dept Astron, Beijing 100871, Peoples R China., Korea Astron & Space Sci Inst 776, Daedeokdae Ro, Daejeon 305348, South Korea., Peking Univ, Hlth Sci Ctr, Xueyuan Rd 38th, Beijing 100191, Peoples R China., Univ Cologne, Inst Phys, Zulpicher Str 77, D-50937 Cologne, Germany., European So Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany.

المصدر: SCI

مصطلحات موضوعية: ISM: abundances, ISM: clouds, ISM: kinematics and dynamics, ISM: molecules, stars: formation, INFRARED DARK CLOUDS, STAR-FORMATION, INTERSTELLAR CLOUDS, PRESTELLAR CORES, HCN, DEPLETION, EMISSION, HERSCHEL, INFLOW, LINE

العلاقة: ASTROPHYSICAL JOURNAL.2016,820,(1).; 1397362; http://hdl.handle.net/20.500.11897/438432Test; WOS:000372787000037

الإتاحة: https://doi.org/20.500.11897/438432Test
https://doi.org/10.3847/0004-637X/820/1/37Test
https://hdl.handle.net/20.500.11897/438432Test

المؤلفون: Zhang, Si-Ju, Wu, Yuefang, Li, Jin Zeng, Yuan, Jing-Hua, Liu, Hong-Li, Dong, Xiaoyi, Huang, Ya-Fang

المساهمون: Wu, YF (reprint author), Peking Univ, Dept Astron, Beijing 100871, Peoples R China., Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing 100012, Peoples R China., Univ Chinese Acad Sci, Beijing 100049, Peoples R China., Peking Univ, Dept Astron, Beijing 100871, Peoples R China.

المصدر: SCI

مصطلحات موضوعية: line: profiles, molecular data, stars: formation, ISM: clouds, ISM: molecules, ISM: structure, BRIGHT-RIMMED CLOUDS, HERBIG-AE/BE STARS, RADIATION-DRIVEN IMPLOSION, YOUNG STELLAR OBJECTS, SPECTRAL ENERGY-DISTRIBUTIONS, INTERMEDIATE-MASS STARS, IRAS POINT SOURCES, H II REGION, FORMING REGIONS, RADIO-CONTINUUM

العلاقة: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY.2016,458,(4),4222-4237.; 1396148; http://hdl.handle.net/20.500.11897/438133Test; WOS:000375799500066

الإتاحة: https://doi.org/20.500.11897/438133Test
https://doi.org/10.1093/mnras/stw597Test
https://hdl.handle.net/20.500.11897/438133Test