| dc.contributor.author | ESPEY, BRIAN RUSSELL | |
| dc.date.accessioned | 2008-06-10T13:09:41Z | |
| dc.date.available | 2008-06-10T13:09:41Z | |
| dc.date.issued | 1994 | |
| dc.date.submitted | 1994 | en |
| dc.identifier.citation | Baker, A. C.; Carswell, R. F.; Bailey, J. A.; Espey, B. R.; Smith, M. G.; Ward, M. J. 'Infrared spectroscopy of high-redshift quasars' in Monthly Notices of the Royal Astronomical Society, 270, (3), 1994, pp. 575 - 579. | en |
| dc.identifier.issn | 51378 | |
| dc.identifier.other | Y | |
| dc.identifier.other | Y | en |
| dc.description | PUBLISHED | en |
| dc.description.abstract | We present H and K spectra (showing redshifted H?, H? and [O III] emission lines) of three radio-loud and three radio-quiet quasars with redshifts z >~ 2, which were obtained using CGS4 on UKIRT The [O III] ?? 4959 + 5007 lines are too weak to allow accurate determination of the redshift of the forbidden lines. The observed Balmer decrements are consistent with enhancement of H? due to collisional excitation. | en |
| dc.format.extent | 575 | en |
| dc.format.extent | 579 | en |
| dc.format.extent | 638930 bytes | |
| dc.format.mimetype | application/pdf | |
| dc.language.iso | en | en |
| dc.relation.ispartofseries | 270 | en |
| dc.relation.ispartofseries | 3 | en |
| dc.rights | Y | en |
| dc.subject | Physics | en |
| dc.title | Infrared spectroscopy of high-redshift quasars | en |
| dc.type | Journal Article | en |
| dc.type.supercollection | scholarly_publications | en |
| dc.type.supercollection | refereed_publications | en |
| dc.identifier.peoplefinderurl | http://people.tcd.ie/espeyb | |
| dc.identifier.rssuri | http://ukads.nottingham.ac.uk/cgi-bin/nph-iarticle_query?1994MNRAS.270..575B&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf | |
| dc.identifier.uri | http://hdl.handle.net/2262/17223 | |
