文章基本信息

标题：The L 1157 protostellar outflow imaged with the Submillimeter Array (Corrigendum)
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作者：A. I. Gómez-Ruiz ; A. I. Gómez-Ruiz ; N. Hirano 等
期刊名称：Astronomy & Astrophysics
印刷版ISSN：0004-6361
电子版ISSN：1432-0746
出版年度：2016
卷号：591
页码：1-2
DOI：10.1051/0004-6361/201118473e
语种：English
出版社：EDP Sciences
摘要：Using the line ratio between the SiO (5–4) and the SiO (2–1) observed by Zhang et al. (2000) with a synthesized beam of 9. ?? 5×8. ?? 0, we derived the physical conditions of the gas in the high-velocity clumps. For our analysis we selected the portion of the high-velocity range that is less affected by the miss- ing flux. The analysis was performed at the B0i and B1a po- sitions, at which the SiO (5–4) emission was detected above the 5σ level. We note that an analysis using several SiO lines ob- served with a single-dish telescope has been made by Nisini et al. (2007). However, they used single-pointing observations, which means that the data were taken with different beam sizes, for instance ∼27 ?? for SiO (2–1) and ∼11 ?? for SiO (5–4). In addi- tion, the line ratios used the total integrated intensity, including the low-velocitycomponent,whereas we used higher-resolution data and focused on the high-velocity component.
关键词：Shock waves;ISM: jets and outflows;Stars: formation;ISM: individual objects: L1157;errata, addenda