Probing the Low-Mass Stellar End of the &eta Chamaeleontis Cluster

Simple item page
dc.contributor.authorSong, Inseok
dc.contributor.authorZuckerman, B
dc.contributor.authorBessell, Michael
dc.date.accessioned2015-12-13T23:11:27Z
dc.date.available2015-12-13T23:11:27Z
dc.date.issued2004
dc.date.updated2015-12-12T08:27:46Z
dc.description.abstractWe have identified three faint new members of the η Chamaeleontis cluster. Spectral types of the new members are estimated to be ∼M5, based on their TiO band strengths and broadband colors. With an age of 5-8 Myr for the cluster, masses of these new me
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/87605
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Open clusters and associations: individual (? Chamaeleontis); Stars: activity; Stars: low-mass, brown dwarfs; Stars: pre-main-sequence
dc.titleProbing the Low-Mass Stellar End of the &eta Chamaeleontis Cluster
dc.typeJournal article
local.bibliographicCitation.lastpage1019
local.bibliographicCitation.startpage1016
local.contributor.affiliationSong, Inseok, Gemini Observatory
local.contributor.affiliationZuckerman, B, University of California
local.contributor.affiliationBessell, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidBessell, Michael, u6900904
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub16962
local.identifier.citationvolume600
local.identifier.doi10.1086/380086
local.identifier.scopusID2-s2.0-1642601964
local.type.statusPublished Version

Downloads

Collections

ANU Research Publications

DSpace software copyright © 2002-2026 LYRASIS