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Disappearance of stellar debris disks around main-sequence stars after 400 million years

Author
HABING, H. J1 ; DOMINIK, C1 ; DE MUIZON, M. J2 3 ; KESSLER, M. F4 ; LAUREIJS, R. J4 ; LEECH, K4 ; METCALFE, L4 ; SALAMA, A4 ; SLEBENMORGEN, R4 ; TRAMS, N4
[1] Leiden Observatory, PO Box 9513, 2300 RA Leiden, Netherlands
[2] DESPA, Observatoire de Paris, 921900 Meudon, France
[3] LAEFF-INTA, ESA Vilspa, PO Box 50727, 28080 Madrid, Spain
[4] Astrophysics Division of ESA, Vilspa, PO Box 50727, 28080, Madrid, Spain
Source

Nature (London). 1999, Vol 401, Num 6752, pp 456-458 ; ref : 22 ref

CODEN
NATUAS
ISSN
0028-0836
Scientific domain
Multidisciplinary
Publisher
Nature Publishing, London
Publication country
United Kingdom
Document type
Article
Language
English
Keyword (fr)
Densité flux Disque circumstellaire Etoile séquence principale Observation IR Poussière circumstellaire
Keyword (en)
Flux density Circumstellar disks Main sequence stars Infrared observation Circumstellar dust
Keyword (es)
Observación IR Polvo circunstelar
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C10 Stellar characteristics and properties / 001E03C10G Accretion and accretion disks

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
1958251

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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