Skip navigation
Skip navigation

Cyanogen in NGC 1851 red giant branch and asymptotic giant branch stars: Quadrimodal distributions

Campbell, S; Yong, David; Wylie de Boer, Elizabeth; Stancliffe, R J; Lattanzio, John; Angelou, G C; D'Orazi, V D; Martell, S L; Grundahl, Frank; Sneden, Chris


The Galactic globular cluster NGC 1851 has raised much interest since Hubble Space Telescope photometry revealed that it hosts a double subgiant branch. Here we report on our homogeneous study into the cyanogen (CN) band strengths in the red giant branch

CollectionsANU Research Publications
Date published: 2012
Type: Journal article
Source: Astrophysical Journal Letters
DOI: 10.1088/2041-8205/761/1/L2
Access Rights: Open Access


File Description SizeFormat Image
01_Campbell_Cyanogen_in_NGC_1851_red_giant_2012.pdf612.53 kBAdobe PDF

Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.

Updated:  17 November 2022/ Responsible Officer:  University Librarian/ Page Contact:  Library Systems & Web Coordinator