On the difference between type E and type A OH/IR stars | |
He JH(何金华)1,2,3; Chen PS(陈培生)1,2,3 | |
刊名 | ASTRONOMICAL JOURNAL |
2001-05 | |
卷号 | 121期号:5页码:2752-2757 |
关键词 | stars : AGB and post-AGB stars : evolution stars : mass loss |
ISSN号 | 0004-6256 |
通讯作者 | He, JH (reprint author), Chinese Acad Sci, Yunnan Observ, Kunming 650011, Peoples R China. |
产权排序 | 第一完成单位 |
英文摘要 | The observed spectral energy distributions of a sample of 60 OH/IR stars are fitted using a radiative transfer model of a dusty envelope. Among the whole sample, 21 stars have reliable phase-lag distances, while the others have less accurate distances. L-*-P, (M) over dot-P, and (M) over dot- L* relations have been plotted for these stars. It is found that type E (with an emission feature at 10 mum) and type A (with an absorption feature at 10 mum) OH/IR stars have different L*P and (M) over dot -L* relations, while both follow a single M-P relation. The type E stars are shown to be located in an area without large-scale dense interstellar medium, while the type A stars are probably located in dense interstellar medium. It is argued here that this may indicate that the two types of OH/IR stars do not share the same chemical composition or zero-age main-sequence mass and so evolve in different ways. This conclusion has reinforced the argument by Chen et al., who reached a similar conclusion from the Galactic distribution of about 1000 OH/IR stars, based on IRAS low-resolution spectrometer spectra. |
学科主题 | Astronomy & Astrophysics |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | OH-IR STARS ; NEAR-INFRARED PHOTOMETRY ; MASS-LOSS ; OPTICAL-PROPERTIES ; SILICATE GRAINS ; GALACTIC-CENTER ; AGB STARS ; GRAPHITE ; MASERS ; RADIO |
收录类别 | SCI |
原文出处 | http://iopscience.iop.org/1538-3881/121/5/2752/ |
语种 | 英语 |
WOS记录号 | WOS:000168592800035 |
内容类型 | 期刊论文 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/4393] |
专题 | 云南天文台_大样本恒星演化研究组 |
作者单位 | 1.Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011, China 2.United Laboratory of Optical Astronomy, CAS 3.National Astronomical Observatories, China |
推荐引用方式 GB/T 7714 | He JH,Chen PS. On the difference between type E and type A OH/IR stars[J]. ASTRONOMICAL JOURNAL,2001,121(5):2752-2757. |
APA | He JH,&Chen PS.(2001).On the difference between type E and type A OH/IR stars.ASTRONOMICAL JOURNAL,121(5),2752-2757. |
MLA | He JH,et al."On the difference between type E and type A OH/IR stars".ASTRONOMICAL JOURNAL 121.5(2001):2752-2757. |
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