WFRF:(Su Bu Mei)
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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 02562naa a2200385 4500 | |
| 001 | oai:DiVA.org:hh-1839 | |
| 003 | SwePub | |
| 008 | 080903s2001 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:hh:diva-18392 URI |
| 024 | 7 | a https://doi.org/10.1016/S0275-1062(01)00039-X2 DOI |
| 040 | a (SwePub)hh | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a art2 swepub-publicationtype |
| 100 | 1 | a Su, Bu-Meiu Yunnan Observatory, Chinese Academy of Sciences, 650011, Kunming, China4 aut |
| 245 | 1 0 | a Sub-milliarcsecond radio structure of three quasars |
| 264 | 1 | b Elsevier,c 2001 |
| 338 | a print2 rdacarrier | |
| 500 | a A translation of Acta Astrophys. Sin. Vol. 20, No. 4 349-354, 2000 | |
| 520 | a The quasars, 0420-014, 0748+126 and 2251+158 (3C 454.3), have been observed at 1.3 cm with a global VLBI network. We have obtained the hybrid maps of the quasars at sub-milliarcsecond resolution. The brightness distribution is revealed in their nuclear regions. The observed data are fitted with a small number of Gaussian components. 2251+158 shows a core-jet structure, and its nuclear region is elongated in the direction PA= -130o. The jet is curved. Its observations at the epoch 1992.9 show it to be in the course of a large burst, accompanied by several smaller ones. The strongest component has a flux of ~ 4.11 Jy (67% of the total detected flux), mostly from an area of 0.16 x 0.01 mas. Doppler boosting is probably responsible for raising the brightness temperature up to 2.6 x 1012 K. | |
| 650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
| 653 | a quasar | |
| 653 | a radio emission | |
| 653 | a sub-milliarcsecond structure | |
| 653 | a Physics | |
| 653 | a Fysik | |
| 700 | 1 | a Li, Yong-Shengu Yunnan Observatory, Chinese Academy of Sciences, 650011, Kunming, China4 aut |
| 700 | 1 | a Bååth, Lars B.u Högskolan i Halmstad,Maskinteknisk produktframtagning (MTEK)4 aut0 (Swepub:hh)baath |
| 700 | 1 | a Gao, Yi-Feiu Yunnan Observatory, Chinese Academy of Sciences, 650011, Kunming, China4 aut |
| 710 | 2 | a Yunnan Observatory, Chinese Academy of Sciences, 650011, Kunming, Chinab Maskinteknisk produktframtagning (MTEK)4 org |
| 773 | 0 | t Chinese Astronomy and Astrophysicsd : Elsevierg 25:1, s. 23-28q 25:1<23-28x 0275-1062x 1879-128X |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:hh:diva-1839 |
| 856 | 4 8 | u https://doi.org/10.1016/S0275-1062(01)00039-X |
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