English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

CCD BVRcIc photometric observations of the 2010 outburst of the recurrentnova U Scorpii are presented. The light-curve has a smooth developmentcharacterized by t2(V)=1.8 and t3(V)=4.1 days, close to the t2(V)=2.2 andt3(V)=4.3 days of 1999 outburst. The plateau phase in 2010 has been brighter,lasting shorter and beginning earlier than in the 1999 outburst. Flickering,with an amplitude twice larger in $I_{\rm C}$ than in $B$ band, was absent onday +4.8 and +15.7, and present on day +11.8, with a time scale of about halfan hour.

BVRcIc photometric evolution and flickering during the 2010 outburst of the recurrent nova U Scorpii