First evidence of dusty disks around Herbig Be stars

被引:50
作者
Fuente, A
Rodríguez-Franco, A
Testi, L
Natta, A
Bachiller, R
Neri, R
机构
[1] Observ Astron Nacl, E-28800 Alcala De Henares, Spain
[2] Univ Complutense Madrid, Dept Matemat Aplicada Biomatemat, E-28037 Madrid, Spain
[3] CSIC, IEM, DAMIR, E-28006 Madrid, Spain
[4] Osserv Astrofis Arcetri, I-50125 Florence, Italy
[5] Inst Radio Astron Millimetr, F-38406 St Martin Dheres, France
关键词
circumstellar matter; radio continuum : stars; stars; individual; (MWC; 137; MWC; 1080; R Monocerotis); stars : pre-main-sequence;
D O I
10.1086/380296
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have carried out a high-sensitivity search for circumstellar disks around Herbig Be stars in the continuum at 1.4 and 2.7 mm using the IRAM interferometer at the Plateau de Bure. In this Letter, we report data on three well-studied B0 stars: MWC 1080, MWC 137, and R Mon. The two latter have also been observed in the continuum at 0.7 and 1.3 cm using the NRAO Very Large Array. We report the detection of circumstellar disks around MWC 1080 and R Mon with masses of M-d similar to 0.003 and 0.01 M-., respectively, while for MWC 137 we estimate a disk mass upper limit of 0.007 M-.. Our results show that the ratio M-d/M-* is at least an order of magnitude lower in Herbig Be stars than in Herbig Ae and T Tauri stars.
引用
收藏
页码:L39 / L42
页数:4
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