A Time‐resolved Photometric Study of the Eclipsing Dwarf Nova RX J0909+1849

2000 ◽  
Vol 112 (777) ◽  
pp. 1467-1478 ◽  
Author(s):  
A. W. Shafter ◽  
L. Lee Clark ◽  
Julia Holland ◽  
Stephen J. Williams



1988 ◽  
Vol 95 ◽  
pp. 178 ◽  
Author(s):  
A. W. Shafter ◽  
F. V. Hessman


2006 ◽  
Vol 2 (S240) ◽  
pp. 536-541
Author(s):  
Akira Imada ◽  
Kaori Kubota ◽  
Taichi Kato ◽  
Daisaku Nogami ◽  
Hiroyuki Maehara ◽  
...  

AbstractWe report on time-resolved CCD photometry of the newly-discovered dwarf nova, TSS J022216.4+412259.9 during its outburst in 2005 November–December. The best-estimated superhump period was 0.0554 days, which is the shortest superhump period among WZ Sge-type dwarf novae ever known. Double-peaked humps were also detected with a period of 0.05487 days in the early stage of the outburst. A rebrightening exhibited after the end of the plateau phase. All of these observations indicate the WZ Sge nature of the system. We mainly discuss the rebrightening stage of the superoutburst, compared with other WZ Sge-type dwarf novae.



1989 ◽  
Vol 240 (4) ◽  
pp. 975-990 ◽  
Author(s):  
J. Echevarria ◽  
F. Diego ◽  
M. Tapia ◽  
R. Costero ◽  
E. Ruiz ◽  
...  


2011 ◽  
Vol 7 (S285) ◽  
pp. 301-302
Author(s):  
Deanne de Budè ◽  
Patrick Woudt ◽  
Brian Warner

AbstractResults of a high-speed photometric study of dwarf novæ in the Catalina Real-time Transient Survey are given. A population of faint dwarf novæ near the orbital period minimum is detected. At the shortest periods there is a correlation between orbital period and outburst interval.



1987 ◽  
Vol 93 ◽  
pp. 125-126
Author(s):  
A.W. Shafter ◽  
J.A. Hill ◽  
E.L. Robinson ◽  
P. Szkody ◽  
J.R. Thorstensen ◽  
...  

AbstractSW UMa is an unusual dwarf nova in several respects. Recent observations by Robinson et al. (1986) have established that SW UMa is an SU UMa system, while Shafter, Szkody, and Thorstensen (1986) have presented evidence suggesting that SW UMa may be a DQ Her system as well. If the DQ Her classification is confirmed then SW UMa will be the only system to have this dual classification. Finally, time resolved spectroscopy of SW UMa has revealed the presence of an S-wave component in the Ha emission which has an unexpected phasing relative to the line wings.



2002 ◽  
Vol 391 (2) ◽  
pp. 565-569 ◽  
Author(s):  
S. V. Antipin ◽  
E. P. Pavlenko
Keyword(s):  


2016 ◽  
Vol 60 (11) ◽  
pp. 971-995 ◽  
Author(s):  
T. S. Khruzina ◽  
I. B. Voloshina ◽  
V. G. Metlov
Keyword(s):  


2003 ◽  
Vol 115 (811) ◽  
pp. 1105-1117 ◽  
Author(s):  
Allen W. Shafter ◽  
Julia N. Holland
Keyword(s):  


1981 ◽  
Vol 248 ◽  
pp. 1067 ◽  
Author(s):  
J. Patterson ◽  
J. T. McGraw ◽  
L. Coleman ◽  
J. L. Africano
Keyword(s):  


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