Stellar Abundances in Giant Stars in the Metal-Rich Globular Cluster NGC 6528
(2003) 296. p.377-378- Abstract
- We present the first results of a detailed abundance analysis, based on VLT observations, of giant stars in the very metal-rich globular cluster NGC 6528. We will be able to tie the horizontal branch abundances (see e.g. Carretta et al. 2001) to those of the more luminous giants (see CMDs). For the very similar cluster NGC 6553 studies of different types of stars have yielded very disparate results. Our first analysis of three of our stars seem to indicate that indeed the different sorts of stars do show similar abundances if one homogeneous set of models and parameters are being used.
Please use this url to cite or link to this publication:
https://lup.lub.lu.se/record/528169
- author
- Feltzing, Sofia LU ; Primas, F. and Johnson, R.
- organization
- publishing date
- 2003
- type
- Chapter in Book/Report/Conference proceeding
- publication status
- published
- subject
- host publication
- New Horizons in Globular Cluster Astronomy (ASP Conference Proceedings ; 296)
- editor
- Piotto, Giampaolo ; Meylan, Georges ; Djorgovski, S. George and Riello, Marco
- volume
- 296
- pages
- 377 - 378
- publisher
- Astronomical Society of the Pacific (ASP)
- external identifiers
-
- wos:000184405600085
- ISBN
- 1-58381-143-5
- language
- English
- LU publication?
- yes
- id
- 6934ad3e-bd2e-4727-b601-3f3923c1619d (old id 528169)
- alternative location
- http://arxiv.org/abs/astro-ph/0211210
- date added to LUP
- 2016-04-04 10:19:01
- date last changed
- 2020-06-16 15:04:59
@inproceedings{6934ad3e-bd2e-4727-b601-3f3923c1619d, abstract = {{We present the first results of a detailed abundance analysis, based on VLT observations, of giant stars in the very metal-rich globular cluster NGC 6528. We will be able to tie the horizontal branch abundances (see e.g. Carretta et al. 2001) to those of the more luminous giants (see CMDs). For the very similar cluster NGC 6553 studies of different types of stars have yielded very disparate results. Our first analysis of three of our stars seem to indicate that indeed the different sorts of stars do show similar abundances if one homogeneous set of models and parameters are being used.}}, author = {{Feltzing, Sofia and Primas, F. and Johnson, R.}}, booktitle = {{New Horizons in Globular Cluster Astronomy (ASP Conference Proceedings ; 296)}}, editor = {{Piotto, Giampaolo and Meylan, Georges and Djorgovski, S. George and Riello, Marco}}, isbn = {{1-58381-143-5}}, language = {{eng}}, pages = {{377--378}}, publisher = {{Astronomical Society of the Pacific (ASP)}}, title = {{Stellar Abundances in Giant Stars in the Metal-Rich Globular Cluster NGC 6528}}, url = {{http://arxiv.org/abs/astro-ph/0211210}}, volume = {{296}}, year = {{2003}}, }