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题名: Evolutionary stages and disk properties of young stellar objects in the Perseus cloud
作者: Zhang, Hong-Xin1, 2, 3, 4, 10; Gao Yu(高煜)5, 6; Fang Min(房敏)5, 7; Yuan, Hai-Bo3; Zhao YingHe(赵应和)5, 6, 8; Chang, Rui-Xiang9; Jiang, Xue-Jian5, 6; Liu, Xiao-Wei3; Luo, A-Li1; Ma HongJun(马红君)5, 6; Shao, Zheng-Yi9; Wang, Xiao-Long5, 6
刊名: RESEARCH IN ASTRONOMY AND ASTROPHYSICS
出版日期: 2015-08-01
卷号: 15, 期号:8, 页码:1294-1324
关键词: stars: formation ; stars: low-mass ; stars: pre-main sequence ; individual: Perseus Cloud ; circumstellar matter ; protoplanetary
学科分类: 天文和天体物理
DOI: 10.1088/1674-4527/15/8/014
文章类型: Article
英文摘要: We investigated the evolutionary stages and disk properties of 211 young stellar objects (YSOs) across the Perseus cloud by modeling their broadband optical to mid-infrared (IR) spectral energy distribution (SED). Our optical gri photometry data were obtained from the recently finished Purple Mountain Observatory Xuyi Schmidt Telescope Photometric Survey of the Galactic Anti-center (XSTPS-GAC). About 81% of our sample fall into the Stage II phase which is characterized by having optically thick disks, while 14% into the Stage I phase characterized by having significant infalling envelopes, and the remaining 5% into the Stage III phase characterized by having optically thin disks. The median stellar age and mass of the Perseus YSOs are 3.1 Myr and 0.3 M-circle dot respectively. By exploring the relationships among the turnoff wave bands lambda(turnoff) (longward of which significant IR excesses above the stellar photosphere are observed), the excess spectral index alpha(excess) as determined for lambda > lambda(turnoff), and the disk inner radius R-in (determined from SED modeling) for YSOs at different evolutionary stages, we found that the median and standard deviation of alpha(excess) for YSOs with optically thick disks tend to increase with lambda(turnoff), especially at lambda(turnoff) >= 5.8 mu m, whereas the median fractional dust luminosities L-dust/L star tend to decrease with increasing lambda(turnoff). This points to an inside-out process of disk clearing for small dust grains. Moreover, a positive correlation between alpha(excess) and R-in was found at alpha(excess) greater than or similar to 0 and R-in greater than or similar to 10 x the dust sublimation radius R-sub, irrespective of lambda(turnoff), L-dust/L star and disk flaring. This suggests that the outer disk flaring either does not evolve synchronously with the inside-out disk clearing of small dust grains or has little appreciable influence on the spectral slopes at lambda less than or similar to 24 mu m. About 23% of our YSO disks are classified as transitional disks, which have lambda(turnoff) = 5.8 mu m and L-dust/L star > 10(-3). The transitional disks and full disks occupy distinctly different regions on the L-dust/L star vs. alpha(excess) diagram. Taking L-dust/L star as an approximate discriminator of disks with (>0.1) and without (<0.1) considerable accretion activity, we found that 65% and 35% of the transitional disks may be consistent with being dominantly cleared by photoevaporation and dynamical interaction with giant planets respectively. None of our transitional disks have alpha(excess) (<0.0) or L-dust/L star (>0.1) values that would otherwise be suggestive of disk clearing dominanted by grain growth.
WOS标题词: Science & Technology ; Physical Sciences
类目[WOS]: Astronomy & Astrophysics
研究领域[WOS]: Astronomy & Astrophysics
关键词[WOS]: LOW-MASS STARS ; SPECTRAL ENERGY-DISTRIBUTIONS ; T-TAURI STARS ; ORION NEBULA CLUSTER ; MAIN-SEQUENCE STARS ; SPITZER C2D SURVEY ; CIRCUMSTELLAR DISKS ; PROTOPLANETARY DISKS ; SUBSTELLAR OBJECTS ; MOLECULAR CLOUD
收录类别: SCI
所属项目名称: PMO_LIB-IR
语种: 英语
WOS记录号: WOS:000360553400014
Citation statistics:
内容类型: 期刊论文
URI标识: http://libir.pmo.ac.cn/handle/332002/14845
Appears in Collections:星系中的恒星形成研究团组_期刊论文

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作者单位: 1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
2.Peking Univ, Dept Astron, Beijing 100871, Peoples R China
3.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China
4.Chinese Acad Sci, South Amer Ctr Astron, Santiago, Chile
5.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China
6.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Jiangsu, Peoples R China
7.Univ Autonoma Madrid, Dept Fis Teor, E-28049 Madrid, Spain
8.CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA
9.Chinese Acad Sci, Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, Shanghai 200030, Peoples R China
10.Pontificia Univ Catolica Chile, Fac Fis, Inst Astrofis, Santiago 7820436, Chile
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