scholarly journals Survey of period variations of superhumps in SU UMa-type dwarf novae. IX. The ninth year (2016–2017)

Author(s):  
Taichi Kato ◽  
Keisuke Isogai ◽  
Franz-Josef Hambsch ◽  
Tonny Vanmunster ◽  
Hiroshi Itoh ◽  
...  
2010 ◽  
Vol 62 (6) ◽  
pp. 1525-1584 ◽  
Author(s):  
Taichi Kato ◽  
Hiroyuki Maehara ◽  
Makoto Uemura ◽  
Arne Henden ◽  
Enrique De Miguel ◽  
...  

2012 ◽  
Vol 64 (1) ◽  
pp. 21 ◽  
Author(s):  
Taichi Kato ◽  
Hiroyuki Maehara ◽  
Ian Miller ◽  
Tomohito Ohshima ◽  
Enrique de Miguel ◽  
...  

2013 ◽  
Vol 65 (1) ◽  
pp. 23 ◽  
Author(s):  
Taichi Kato ◽  
Franz-Josef Hambsch ◽  
Hiroyuki Maehara ◽  
Gianluca Masi ◽  
Ian Miller ◽  
...  

2016 ◽  
Vol 68 (4) ◽  
pp. 65 ◽  
Author(s):  
Taichi Kato ◽  
Franz-Josef Hambsch ◽  
Berto Monard ◽  
Tonny Vanmunster ◽  
Yutaka Maeda ◽  
...  

Author(s):  
Taichi Kato ◽  
Pavol A. Dubovsky ◽  
Igor Kudzej ◽  
Franz-Josef Hambsch ◽  
Ian Miller ◽  
...  

2014 ◽  
Vol 66 (2) ◽  
pp. 30 ◽  
Author(s):  
Taichi Kato ◽  
Franz-Josef Hambsch ◽  
Hiroyuki Maehara ◽  
Gianluca Masi ◽  
Francesca Nocentini ◽  
...  

Author(s):  
Taichi Kato ◽  
Keisuke Isogai ◽  
Yasuyuki Wakamatsu ◽  
Franz-Josef Hambsch ◽  
Hiroshi Itoh ◽  
...  

Abstract Continuing the project described by Kato et al. (2009, PASJ, 61, S395), we collected times of superhump maxima for 102 SU UMa-type dwarf novae observed mainly during the 2017 season, and characterized these objects. WZ Sge-type stars identified in this study are PT And, ASASSN-17ei, ASASSN-17el, ASASSN-17es, ASASSN-17fn, ASASSN-17fz, ASASSN-17hw, ASASSN-17kd, ASASSN-17la, PNV J20205397$+$2508145, and TCP J00332502$-$3518565. We obtained new mass ratios for seven objects using growing superhumps (stage A). ASASSN-17gf is an EI Psc-type object below the period minimum. CRTS J080941.3$+$171528 and DDE 51 are objects in the period gap, and both showed a long-lasting phase of stage A superhumps. We also summarize the recent advances in understanding of SU UMa-type and WZ Sge-type dwarf novae.


2009 ◽  
Vol 61 (sp2) ◽  
pp. S395-S616 ◽  
Author(s):  
Taichi Kato ◽  
Akira Imada ◽  
Makoto Uemura ◽  
Daisaku Nogami ◽  
Hiroyuki Maehara ◽  
...  

2015 ◽  
Vol 67 (6) ◽  
pp. 105 ◽  
Author(s):  
Taichi Kato ◽  
Franz-Josef Hambsch ◽  
Pavol A. Dubovsky ◽  
Igor Kudzej ◽  
Berto Monard ◽  
...  

1966 ◽  
Vol 25 ◽  
pp. 197-222 ◽  
Author(s):  
P. J. Message

An analytical discussion of that case of motion in the restricted problem, in which the mean motions of the infinitesimal, and smaller-massed, bodies about the larger one are nearly in the ratio of two small integers displays the existence of a series of periodic solutions which, for commensurabilities of the typep+ 1:p, includes solutions of Poincaré'sdeuxième sortewhen the commensurability is very close, and of thepremière sortewhen it is less close. A linear treatment of the long-period variations of the elements, valid for motions in which the elements remain close to a particular periodic solution of this type, shows the continuity of near-commensurable motion with other motion, and some of the properties of long-period librations of small amplitude.To extend the investigation to other types of motion near commensurability, numerical integrations of the equations for the long-period variations of the elements were carried out for the 2:1 interior case (of which the planet 108 “Hecuba” is an example) to survey those motions in which the eccentricity takes values less than 0·1. An investigation of the effect of the large amplitude perturbations near commensurability on a distribution of minor planets, which is originally uniform over mean motion, shows a “draining off” effect from the vicinity of exact commensurability of a magnitude large enough to account for the observed gap in the distribution at the 2:1 commensurability.


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