SIMBAD references

2004ApJ...600.1016S - Astrophys. J., 600, 1016-1019 (2004/January-2)

Probing the low-mass stellar end of the η Chamaeleontis cluster.

SONG I., ZUCKERMAN B. and BESSELL M.S.

Abstract (from CDS):

We 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 members are estimated to be ∼0.08 M. All three display strong Li 6708 Å absorption and Hα emission features, including one with an Hα emission equivalent width of ∼60 Å, along with He I 6678 and 7605 Å emission features that are characteristics of classical T Tauri stars.

Abstract Copyright:

Journal keyword(s): Galaxy: Open Clusters and Associations: Individual: Name: η Chamaeleontis - Stars: Activity - Stars: Low-Mass, Brown Dwarfs - Stars: Pre-Main-Sequence

Nomenclature: Table 2: ECHA JHHMM.m+DDMM N=4 added.

Simbad objects: 26

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2004ApJ...600.1016S and select 'bookmark this link' or equivalent in the popup menu


2021.06.15-09:09:39

© Université de Strasbourg/CNRS

    • Contact