As reported on VSNET (Kato, vsnet-alert 10399), the infrequently
outbursting dwarf nova HO Del is in superoutburst for the first
time since 2001. Observations submitted to the AAVSO indicate
the star is currently near m(vis) ~ 14.7 (Gary Poyner, JD
2454682.485), and likely went into outburst some time between
JD 2454680.43 (Eddy Muyllaert, m(vis) < 14.4) and JD 2454681.49
(Hubert Hautecler, m(vis) = 14.2).
Kato et al (2003; PASJ 55, 989) showed that this star has several
peculiarities among the SU UMa stars, including: peculiar superhump
behavior; a low outburst amplitude relative to other long
recurrence-time SU UMa stars; and a high X-ray luminosity.
Visual observations and instrumental time-series photometry
of HO Del are encouraged.
HO Del is located at RA: 20 36 55.50 , Dec: +14 03 10.0 (J2000)
Charts and sequence photometry for HO Del are available via VSP:
http://www.aavso.org/observing/charts/vsp/index.html?pickname=HO%20Del
Please submit data to the AAVSO as "HO Del" (AUID 000-BCL-980).
This AAVSO Special Notice was prepared by Matthew Templeton.
---------------------------------------------------
SUBMIT OBSERVATIONS TO THE AAVSO
Information on submitting observations to the AAVSO may be found at:
http://www.aavso.org/observing/submit/
SPECIAL NOTICE ARCHIVE AND SUBSCRIPTION INFORMATION
A Special Notice archive is available at the following URL:
http://www.aavso.org/publications/specialnotice/
Subscribing and Unsubscribing may be done at the following URL:
http://www.aavso.org/publications/email/