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Millimetre Observations of Infrared Carbon Stars. II. Mass loss rates and expansion velocities

dc.contributor.authorGroenewegen, M A T
dc.contributor.authorSevenster, Maartje N
dc.contributor.authorSpoon, H W W
dc.contributor.authorPerez, I
dc.date.accessioned2015-12-13T22:28:49Z
dc.date.available2015-12-13T22:28:49Z
dc.date.issued2002
dc.date.updated2015-12-11T08:42:02Z
dc.description.abstractDust- and gas mass loss rates and distances are determined for a sample of about 330 infra-red carbon stars that probe a distance up to about 5.5 kpc. The dependence of the dust- and gas mass loss rates, and the expansion velocity upon galactic longitude
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/74380
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.subjectKeywords: Bolometers; Dust; Galaxies; High frequency telecommunication lines; Radio astronomy; Carbon stars; Astrophysics Circumstellar matter; Radio lines: stars; Stars: AGB and post-AGB; Stars: mass loss
dc.titleMillimetre Observations of Infrared Carbon Stars. II. Mass loss rates and expansion velocities
dc.typeJournal article
local.bibliographicCitation.lastpage522
local.bibliographicCitation.startpage511
local.contributor.affiliationGroenewegen, M A T, University of Leuven
local.contributor.affiliationSevenster, Maartje N, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationSpoon, H W W, University of Groningen Kapteyn Astronomical Institute
local.contributor.affiliationPerez, I, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidSevenster, Maartje N, u9807734
local.contributor.authoruidPerez, I, u2505257
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub4094
local.identifier.citationvolume390
local.identifier.scopusID2-s2.0-0036682438
local.type.statusPublished Version

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