Fullerenes in the circumstellar medium of Herbig Ae/Be stars: insights from the Spitzer mid-infrared spectral catalog

被引:2
|
作者
Arun, R. [1 ,2 ]
Mathew, Blesson [2 ]
Manoj, P. [3 ]
Maheswar, G. [1 ]
Shridharan, B. [2 ]
Kartha, Sreeja S. [2 ]
Narang, Mayank [3 ,4 ]
机构
[1] Indian Inst Astrophys, Sarjapur Rd, Bangalore 560034, India
[2] CHRIST Deemed Univ, Dept Phys & Elect, Bangalore 560029, India
[3] Tata Inst Fundamental Res, Homi Bhabha Rd, Mumbai 400005, India
[4] Acad Sinica, Inst Astron & Astrophys, 1 Sect 4, Roosevelt Rd, Taipei 10617, Taiwan
关键词
astrochemistry; stars: variables: T Tauri; Herbig Ae/Be; ISM: molecules; infrared: general; YOUNG STELLAR OBJECTS; POLYCYCLIC AROMATIC-HYDROCARBONS; INFRARED-EMISSION BANDS; MU-M EMISSION; INTERSTELLAR EXTINCTION; ENERGY-DISTRIBUTIONS; FORMING REGIONS; CORNELL ATLAS; X-SHOOTER; POST-AGB;
D O I
10.1093/mnras/stad1511
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This study presents the largest mid-infrared spectral catalogue of Herbig Ae/Be stars to date, containing the Spitzer Infrared Spectrograph spectra of 126 stars. Based on the catalogue analysis, two prominent infrared vibrational modes of C-60 bands at 17.4 and 18.9 mu m are detected in the spectra of nine sources, while 7.0 mu m feature is identified in the spectra of HD 319896. The spectral index analysis and the comparison of the known sources with C-60 features indicated that there exist two different types of emission classes among the sample of stars. The infrared spectra of six Herbig Ae/Be stars in this study resemble that of reflection nebulae, and their association with previously known reflection nebulae is confirmed. In the case of three Herbig Ae/Be stars, we report the tentative evidence of C-60 emission features originating from the circumstellar disc or nearby diffused emission region. The detection fraction of C-60 in the total HAeBe star sample is similar to 7 per cent, whereas the detection fraction is 30 per cent for HAeBe stars associated with nebulosity. In the catalog, C-60 is exclusively present in the circumstellar regions of B type Herbig Ae/Be stars, with no evidence of its presence detected in stars with later spectral types. The present study has increased the number of young stellar objects and reflection nebulae detected with C-60 multifold, which can help in understanding the excitation and formation pathway of the species.
引用
收藏
页码:1601 / 1613
页数:13
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