The Slow Late Decline of the Old Nova RW Ursae Minoris (1956)

dc.contributor.author	DI MILLE, F.
dc.contributor.author	Alis, S.
dc.contributor.author	TAMBURINI, F.
dc.contributor.author	Saygac, Ahmet Talat
dc.contributor.author	Bianchini, A.
dc.date.accessioned	2021-03-05T15:12:11Z
dc.date.available	2021-03-05T15:12:11Z
dc.identifier.citation	Bianchini A., DI MILLE F., TAMBURINI F., Saygac A. T. , Alis S., "The Slow Late Decline of the Old Nova RW Ursae Minoris (1956)", 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.221-224
dc.identifier.other	vv_1032021
dc.identifier.other	av_bac96afc-8d56-43b9-8671-762f6708555c
dc.identifier.uri	http://hdl.handle.net/20.500.12627/124227
dc.description.abstract	Photometric observations of the old nova RW UMi are presented. Data obtained mostly in the Asiago Observatory of lNAF. The period analysis of the data did not permit to recover the Retter & Lipkin (2001) period. A possible explanation to the nature of QPO in the data is given.
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	The Slow Late Decline of the Old Nova RW Ursae Minoris (1956)
dc.type	Bildiri
dc.contributor.department	University of Padua , ,
dc.identifier.volume	490
dc.contributor.firstauthorID	20801

Bu öğenin dosyaları:

Dosyalar	Boyut	Biçim	Göster
Bu öğe ile ilişkili dosya yok.