dc.contributor.author |
Suleimanov V. |
|
dc.contributor.author |
Neustroev V. |
|
dc.contributor.author |
Borisov N. |
|
dc.contributor.author |
Fioktistova I. |
|
dc.date.accessioned |
2018-09-17T21:32:36Z |
|
dc.date.available |
2018-09-17T21:32:36Z |
|
dc.date.issued |
2004 |
|
dc.identifier.issn |
1405-2059 |
|
dc.identifier.uri |
https://dspace.kpfu.ru/xmlui/handle/net/135128 |
|
dc.description.abstract |
Medium resolution spectroscopy of nova-like cataclysmic variable UX UMA was performed using the 6-m telescope SAO RAS in April 1999. Obtained spectra cover the total orbital period including eclipse phases and allow us to reproduce the radial velocity curve. The radial-velocity variations of the Hβ emission line are found to have semi-amplitude of about 100 km/s. © Copyright 2004: IA, UNAM. |
|
dc.relation.ispartofseries |
Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias |
|
dc.title |
Time-resolved spectroscopy and doppler tomography of UX UMa |
|
dc.type |
Conference Paper |
|
dc.relation.ispartofseries-volume |
20 |
|
dc.collection |
Публикации сотрудников КФУ |
|
dc.relation.startpage |
270 |
|
dc.source.id |
SCOPUS14052059-2004-20-SID33846018746 |
|