| dc.contributor.author | Weilbacher, P. | |
| dc.contributor.author | Fritze, U. | |
| dc.contributor.author | Duc, P.A. | |
| dc.date.accessioned | 2009-04-27T08:47:48Z | |
| dc.date.available | 2009-04-27T08:47:48Z | |
| dc.date.issued | 2003 | |
| dc.identifier.citation | Weilbacher , P , Fritze , U & Duc , P A 2003 , ' Optical and NIR investigation of a sample of tidal dwarf candidates ' , Astrophysics and Space Science , vol. 284 , no. 2 , pp. 639-642 . https://doi.org/10.1023/A:1024082728293 | |
| dc.identifier.issn | 0004-640X | |
| dc.identifier.other | PURE: 165687 | |
| dc.identifier.other | PURE UUID: 3256726f-f90a-4798-9ac7-06e6937e85cd | |
| dc.identifier.other | dspace: 2299/3299 | |
| dc.identifier.other | Scopus: 0347758348 | |
| dc.identifier.uri | http://hdl.handle.net/2299/3299 | |
| dc.description | “The original publication is available at www.springerlink.com”. Copyright Springer. [Full text of this article is not available in the UHRA] | |
| dc.description.abstract | We analyzed a sample of 44 candidates for Tidal Dwarf Galaxies(TDGs) previously selected on optical imaging with low resolution spectroscopy. Most of the TDG candidates have the same redshift as the interacting system, 3 of them very likely are low metallicity dwarf galaxies in projection, and 13 show signs of kinematics decoupled from their hosting tidal tail. Subsequent NIR photometry in combination with evolutionary synthesis modeling allows us to derive stellar masses, star formation rates, and the ratio of old to young stars within each TDG candidate. | en |
| dc.language.iso | eng | |
| dc.relation.ispartof | Astrophysics and Space Science | |
| dc.title | Optical and NIR investigation of a sample of tidal dwarf candidates | en |
| dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
| dc.description.status | Peer reviewed | |
| rioxxterms.versionofrecord | https://doi.org/10.1023/A:1024082728293 | |
| rioxxterms.type | Journal Article/Review | |
| herts.preservation.rarelyaccessed | true | |
