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First Evidence of Dusty Disks around Herbig Be Stars

A. Fuente et al 2003 ApJ 598 L39-L42   doi: 10.1086/380296  Help

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A. Fuente1, A. Rodríguez-Franco2,3, L. Testi4, A. Natta4, R. Bachiller1 and R. Neri5
1 Observatorio Astronómico Nacional, Apartado 1143, E-28800 Alcalá de Henares, Spain
2 Departamento Matemática Aplicada (Biomatemática), Universidad Complutense de Madrid, Avenida Arcos de Jalón s/n, E-28037 Madrid, Spain
3 Consejo Superior de Investigaciones Científicas, IEM, DAMIR, Serrano 121, E-28006 Madrid, Spain
4 Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, I-50125 Firenze, Italy
5 Institut de Radioastronomie Millimétrique, 300 rue de la Piscine, 38406 St. Martin d'Hères Cedex, France
E-mail: a.fuente@oan.es

ABSTRACT. 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 Md ~ 0.003 and 0.01 Msun, respectively, while for MWC 137 we estimate a disk mass upper limit of 0.007 Msun. Our results show that the ratio Md/M* is at least an order of magnitude lower in Herbig Be stars than in Herbig Ae and T Tauri stars.

Subject headings: circumstellar matter; radio continuum: stars; stars: individual (MWC 137, MWC 1080, R Monocerotis); stars: pre-main sequence

Print publication: Issue 1 (2003 November 20)
Received 2003 July 9, accepted for publication 2003 October 1
Published 2003 November 3

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