A mid-infrared interferometric study of the circumstellar environment of dusty oh/ir stars with vlti/midi

T. Driebe; K. Ohnaka; K. Murakawa; K. H. Hofmann; D. Schertl; G. Weigelt; T. Verhoelst; O. Chesneau; A. Domiciano De Souza; D. Riechers; M. Schöller; M. Wittkowski

doi:10.1007/978-1-4020-9190-2_21

A mid-infrared interferometric study of the circumstellar environment of dusty oh/ir stars with vlti/midi

T. Driebe, K. Ohnaka, K. Murakawa, K. H. Hofmann, D. Schertl, G. Weigelt, T. Verhoelst, O. Chesneau, A. Domiciano De Souza, D. Riechers, M. Schöller, M. Wittkowski

Resultado de la investigación: Contribución a los tipos de informe/libro › Contribución a la conferencia › revisión exhaustiva

Resumen

OH/IR stars are evolved stars exhibiting large infrared excess as well as prominent OH maser emission. The vast majority of this heterogeneous object class are highly-evolved low- and intermediate-mass stars ascending the upper part of the asymptotic giant branch (AGB). Thus, these stars are in the final phase of their AGB evolution which is characterized by intensive mass loss with mass-loss rates that can reach up to 10⁻⁴ M_⊙. This high mass loss leads to the development of an extended, usually optically thick dusty circumstellar envelope which can be well studied with infrared-interferometric observations.

Idioma original	Inglés
Título de la publicación alojada	Astrophysics and Space Science Proceedings
Editores	Alan Moorwood
Editorial	Springer Science and Business Media B.V.
Páginas	125-126
Número de páginas	2
Edición	202459
ISBN (versión digital)	9781402091902
ISBN (versión impresa)	9780387727677, 9780387876207, 9781402055720, 9781402069321, 9781402088674, 9781402091896, 9781402091896, 9781441981608, 9781441983688, 9783540758259, 9783642033230, 9783642103216, 9783642103513, 9783642113406, 9783642172502, 9789048133994, 9789048134984
DOI	https://doi.org/10.1007/978-1-4020-9190-2_21
Estado	Publicada - 2009
Publicado de forma externa	Sí
Evento	Workshop on Science with the VLT in the ELT Era, 2007 - Garching, Alemania Duración: 8 oct. 2007 → 12 oct. 2007

Serie de la publicación

Nombre	Astrophysics and Space Science Proceedings
Número	202459
Volumen	0
ISSN (versión impresa)	1570-6591
ISSN (versión digital)	1570-6605

Conferencia

Conferencia	Workshop on Science with the VLT in the ELT Era, 2007
País/Territorio	Alemania
Ciudad	Garching
Período	8/10/07 → 12/10/07

Áreas temáticas de ASJC Scopus

Física y astronomía (todo)
Informática aplicada
Espectroscopia
Ciencias planetarias y espacial
Física nuclear y de alta energía

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10.1007/978-1-4020-9190-2_21

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Driebe, T., Ohnaka, K., Murakawa, K., Hofmann, K. H., Schertl, D., Weigelt, G., Verhoelst, T., Chesneau, O., Domiciano De Souza, A., Riechers, D., Schöller, M., & Wittkowski, M. (2009). A mid-infrared interferometric study of the circumstellar environment of dusty oh/ir stars with vlti/midi. En A. Moorwood (Ed.), Astrophysics and Space Science Proceedings (202459 ed., pp. 125-126). (Astrophysics and Space Science Proceedings; Vol. 0, N.º 202459). Springer Science and Business Media B.V.. https://doi.org/10.1007/978-1-4020-9190-2_21

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title = "A mid-infrared interferometric study of the circumstellar environment of dusty oh/ir stars with vlti/midi",

abstract = "OH/IR stars are evolved stars exhibiting large infrared excess as well as prominent OH maser emission. The vast majority of this heterogeneous object class are highly-evolved low- and intermediate-mass stars ascending the upper part of the asymptotic giant branch (AGB). Thus, these stars are in the final phase of their AGB evolution which is characterized by intensive mass loss with mass-loss rates that can reach up to 10−4 M⊙. This high mass loss leads to the development of an extended, usually optically thick dusty circumstellar envelope which can be well studied with infrared-interferometric observations.",

author = "T. Driebe and K. Ohnaka and K. Murakawa and Hofmann, {K. H.} and D. Schertl and G. Weigelt and T. Verhoelst and O. Chesneau and {Domiciano De Souza}, A. and D. Riechers and M. Sch{\"o}ller and M. Wittkowski",

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doi = "10.1007/978-1-4020-9190-2_21",

language = "English",

isbn = "9780387727677",

series = "Astrophysics and Space Science Proceedings",

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Driebe, T, Ohnaka, K, Murakawa, K, Hofmann, KH, Schertl, D, Weigelt, G, Verhoelst, T, Chesneau, O, Domiciano De Souza, A, Riechers, D, Schöller, M & Wittkowski, M 2009, A mid-infrared interferometric study of the circumstellar environment of dusty oh/ir stars with vlti/midi. En A Moorwood (ed.), Astrophysics and Space Science Proceedings. 202459 ed., Astrophysics and Space Science Proceedings, n.º 202459, vol. 0, Springer Science and Business Media B.V., pp. 125-126, Workshop on Science with the VLT in the ELT Era, 2007, Garching, Alemania, 8/10/07. https://doi.org/10.1007/978-1-4020-9190-2_21

A mid-infrared interferometric study of the circumstellar environment of dusty oh/ir stars with vlti/midi. / Driebe, T.; Ohnaka, K.; Murakawa, K. et al.

Astrophysics and Space Science Proceedings. ed. / Alan Moorwood. 202459. ed. Springer Science and Business Media B.V., 2009. p. 125-126 (Astrophysics and Space Science Proceedings; Vol. 0, N.º 202459).

Resultado de la investigación: Contribución a los tipos de informe/libro › Contribución a la conferencia › revisión exhaustiva

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AU - Murakawa, K.

AU - Hofmann, K. H.

AU - Schertl, D.

AU - Weigelt, G.

AU - Verhoelst, T.

AU - Chesneau, O.

AU - Domiciano De Souza, A.

AU - Riechers, D.

AU - Schöller, M.

AU - Wittkowski, M.

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AB - OH/IR stars are evolved stars exhibiting large infrared excess as well as prominent OH maser emission. The vast majority of this heterogeneous object class are highly-evolved low- and intermediate-mass stars ascending the upper part of the asymptotic giant branch (AGB). Thus, these stars are in the final phase of their AGB evolution which is characterized by intensive mass loss with mass-loss rates that can reach up to 10−4 M⊙. This high mass loss leads to the development of an extended, usually optically thick dusty circumstellar envelope which can be well studied with infrared-interferometric observations.

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ER -

Driebe T, Ohnaka K, Murakawa K, Hofmann KH, Schertl D, Weigelt G et al. A mid-infrared interferometric study of the circumstellar environment of dusty oh/ir stars with vlti/midi. En Moorwood A, editor, Astrophysics and Space Science Proceedings. 202459 ed. Springer Science and Business Media B.V. 2009. p. 125-126. (Astrophysics and Space Science Proceedings; 202459). doi: 10.1007/978-1-4020-9190-2_21

A mid-infrared interferometric study of the circumstellar environment of dusty oh/ir stars with vlti/midi

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Conferencia

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