The Orbital Period of Nova Aquilae 1999 No. 2 (V1494 Aql)статья
Информация о цитировании статьи получена из
Web of Science,
Scopus
Статья опубликована в журнале из списка Web of Science и/или Scopus
Дата последнего поиска статьи во внешних источниках: 18 декабря 2013 г.
Аннотация:The photometric monitoring of Nova V1494 Aql at the Sternberg Astronomical Institute and at the Special Astrophysical Observatory in July and September 2002 has confirmed that the star is an eclipsing system. Its orbital period was improved, 0.1346141(5) days. Light elements and eight mid-eclipse times are given. The light-curve shape suggests that the star is an intermediate polar.