| dc.contributor.author | Saygac, Ahmet Talat | |
| dc.contributor.author | Alis, Sinan | |
| dc.date.accessioned | 2021-03-03T20:58:11Z | |
| dc.date.available | 2021-03-03T20:58:11Z | |
| dc.identifier.citation | Alis S., Saygac A. T. , "Investigating the Nova Rate Connection to Galaxy Type using Archival Hubble Space Telescope Images", 4th International Conference on Classical and Recurrent Novae - Stella Novae: Past and Future Decades, Cape-Town, Güney Afrika, 4 - 08 Şubat 2013, cilt.490, ss.95-98 | |
| dc.identifier.other | vv_1032021 | |
| dc.identifier.other | av_5cc1293c-8e14-479a-a5cd-69d3d77c9aee | |
| dc.identifier.uri | http://hdl.handle.net/20.500.12627/65009 | |
| dc.description.abstract | An attempt to test the nova rate dependency on galaxy type has been made using archival HST data. 41 novae were detected in 17 galaxies beyond the Local Group. Thus it was possible to compute luminosity specific nova rates for 15 galaxies where only one of them (M100) had a previously measured nova rate. | |
| dc.language.iso | eng | |
| dc.subject | Temel Bilimler | |
| dc.subject | Fizik | |
| dc.subject | Astronomi ve Astrofizik | |
| dc.subject | Temel Bilimler (SCI) | |
| dc.subject | Uzay bilimi | |
| dc.subject | ASTRONOMİ VE ASTROFİZİK | |
| dc.title | Investigating the Nova Rate Connection to Galaxy Type using Archival Hubble Space Telescope Images | |
| dc.type | Bildiri | |
| dc.contributor.department | İstanbul Üniversitesi , , | |
| dc.identifier.volume | 490 | |
| dc.contributor.firstauthorID | 20798 | |
