| dc.creator | YALIA DIVAKARA MAYYA | |
| dc.date | 2007 | |
| dc.date.accessioned | 2023-07-25T16:22:46Z | |
| dc.date.available | 2023-07-25T16:22:46Z | |
| dc.identifier | http://inaoe.repositorioinstitucional.mx/jspui/handle/1009/980 | |
| dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/7806180 | |
| dc.description | We investigate the correlation between the bulge effective radius (re ) and disk scale length (rd ) in the near-infrared K band for lenticular galaxies in the field and in clusters. We find markedly different relations between the two parameters as a function of luminosity. Lenticulars with total absolute magnitude fainter than MT =-24.5 show a positive correlation, in line with predictions of secular formation processes for the pseudobulges of late-type disk galaxies. But brighter lenticulars with MT <-24.5 show an anticorrelation, indicating that they
formed through a different mechanism. The available data are insufficient to reliably determine the effect of galaxy environment on these correlations. | |
| dc.format | application/pdf | |
| dc.language | eng | |
| dc.publisher | The astrophysical journal | |
| dc.relation | citation:Barway, Sudhanshu., et al., (2007). Lenticular galaxy formation: possible luminosity dependence, The Astrophysical Journal, Vol.661(1): L37–L40 | |
| dc.rights | info:eu-repo/semantics/openAccess | |
| dc.rights | http://creativecommons.org/licenses/by-nc-nd/4.0 | |
| dc.subject | info:eu-repo/classification/cti/1 | |
| dc.subject | info:eu-repo/classification/cti/21 | |
| dc.subject | info:eu-repo/classification/cti/21 | |
| dc.title | Lenticular galaxy formation: possible luminosity dependence | |
| dc.type | info:eu-repo/semantics/article | |
| dc.type | info:eu-repo/semantics/acceptedVersion | |
| dc.audience | students | |
| dc.audience | researchers | |
| dc.audience | generalPublic | |
