| dc.contributor.author | Viljoen, D.N. | |
| dc.contributor.author | Loubser, S.I. | |
| dc.date.accessioned | 2016-11-08T11:13:20Z | |
| dc.date.available | 2016-11-08T11:13:20Z | |
| dc.date.issued | 2012 | |
| dc.identifier.citation | Viljoen, D.N. & Loubser, S.I. 2012. Did brightest cluster galaxies experience more than one star formation epoch? Proceedings of the International Astronomical Union, 8(295):320. [https://doi.org/10.1017/S174392131300522X] | en_US |
| dc.identifier.issn | 1743-9213 | |
| dc.identifier.issn | 1743-9221 (Online) | |
| dc.identifier.uri | http://hdl.handle.net/10394/19347 | |
| dc.identifier.uri | https://doi.org/10.1017/S174392131300522X | |
| dc.identifier.uri | http://journals.cambridge.org/article_S174392131300522X | |
| dc.description.abstract | We use the full spectrum fitting ability of ULySS, with the Pegase.HR stellar population
model to fit the observed spectra of 40 brightest cluster galaxies in order to determine
whether a single or a composite stellar population provided the most probable representation of
the star formation history (SFH). We find that some galaxies in the sample have more complex
SFHs | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | Cambridge University Press | en_US |
| dc.subject | Galaxies: evolution | en_US |
| dc.subject | Galaxies: general | en_US |
| dc.subject | Galaxies: stellar content | en_US |
| dc.title | Did brightest cluster galaxies experience more than one star formation epoch? | en_US |
| dc.type | Presentation | en_US |
| dc.contributor.researchID | 11290471 - Loubser, Susan Ilani | |
