Prevalence of SED Turndown among Classical Be Stars: Are All Be Stars Close Binaries?

Robert Klement; A.~C. Carciofi; T. Rivinius; R. Ignace; L.~D. Matthews; K. Torstensson; D. Gies; R.~G. Vieira; N.~D. Richardson; A. Domiciano de Souza; J.~E. Bjorkman; G. Hallinan; D.~M. Faes; B. Mota; A.~D. Gullingsrud; C. de Breuck; P. Kervella; M. Curé; D. Gunawan

doi:10.3847/1538-4357/ab48e7

Prevalence of SED Turndown among Classical Be Stars: Are All Be Stars Close Binaries?

Robert Klement, A.~C. Carciofi, T. Rivinius, R. Ignace, L.~D. Matthews, K. Torstensson, D. Gies, R.~G. Vieira, N.~D. Richardson, A. Domiciano de Souza, J.~E. Bjorkman, G. Hallinan, D.~M. Faes, B. Mota, A.~D. Gullingsrud, C. de Breuck, P. Kervella, M. Curé, D. Gunawan

Physics & Astronomy

Research output: Contribution to journal › Article › peer-review

Original language	Undefined/Unknown
Pages (from-to)	147
Number of pages	1
Journal	Astrophysical Journal
Volume	885
Issue number	2
DOIs	https://doi.org/10.3847/1538-4357/ab48e7
State	Published - Nov 1 2019

Keywords

Be stars
Circumstellar disks
Binary stars
Radio continuum emission
Early-type emission stars
Stellar rotation
Stellar evolution
Infrared excess
Stellar astronomy
Circumstellar matter
Radio astronomy
Subdwarf stars
142
235
154
1340
428
1629
1599
788
1583
241
1338
2054
Astrophysics - Solar and Stellar Astrophysics

Access to Document

10.3847/1538-4357/ab48e7

Cite this

Klement, R., Carciofi, A. C., Rivinius, T., Ignace, R., Matthews, L. D., Torstensson, K., Gies, D., Vieira, R. G., Richardson, N. D., Domiciano de Souza, A., Bjorkman, J. E., Hallinan, G., Faes, D. M., Mota, B., Gullingsrud, A. D., de Breuck, C., Kervella, P., Curé, M., & Gunawan, D. (2019). Prevalence of SED Turndown among Classical Be Stars: Are All Be Stars Close Binaries? Astrophysical Journal, 885(2), 147. https://doi.org/10.3847/1538-4357/ab48e7

Klement, R, Carciofi, AC, Rivinius, T, Ignace, R, Matthews, LD, Torstensson, K, Gies, D, Vieira, RG, Richardson, ND, Domiciano de Souza, A, Bjorkman, JE, Hallinan, G, Faes, DM, Mota, B, Gullingsrud, AD, de Breuck, C, Kervella, P, Curé, M & Gunawan, D 2019, 'Prevalence of SED Turndown among Classical Be Stars: Are All Be Stars Close Binaries?', Astrophysical Journal, vol. 885, no. 2, pp. 147. https://doi.org/10.3847/1538-4357/ab48e7

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title = "Prevalence of SED Turndown among Classical Be Stars: Are All Be Stars Close Binaries?",

keywords = "Be stars, Circumstellar disks, Binary stars, Radio continuum emission, Early-type emission stars, Stellar rotation, Stellar evolution, Infrared excess, Stellar astronomy, Circumstellar matter, Radio astronomy, Subdwarf stars, 142, 235, 154, 1340, 428, 1629, 1599, 788, 1583, 241, 1338, 2054, Astrophysics - Solar and Stellar Astrophysics",

author = "Robert Klement and A.\textasciitilde{}C. Carciofi and T. Rivinius and R. Ignace and L.\textasciitilde{}D. Matthews and K. Torstensson and D. Gies and R.\textasciitilde{}G. Vieira and N.\textasciitilde{}D. Richardson and \{Domiciano de Souza\}, A. and J.\textasciitilde{}E. Bjorkman and G. Hallinan and D.\textasciitilde{}M. Faes and B. Mota and A.\textasciitilde{}D. Gullingsrud and \{de Breuck\}, C. and P. Kervella and M. Cur{\'e} and D. Gunawan",

year = "2019",

month = nov,

day = "1",

doi = "10.3847/1538-4357/ab48e7",

language = "Undefined/Unknown",

volume = "885",

pages = "147",

journal = "Astrophysical Journal",