Fig. 6.
Light curve of NY Ser in 2018 reproduced from figure 1 in Kato et al. (2018). The abscissa is in BJD−2400000. This SU UMa-type dwarf nova showed standstills which were terminated by superoutbursts (SO1 and SO2). (Color online)

Light curve of NY Ser in 2018 reproduced from figure 1 in Kato et al. (2018). The abscissa is in BJD−2400000. This SU UMa-type dwarf nova showed standstills which were terminated by superoutbursts (SO1 and SO2). (Color online)

Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close