Rx J1015.5+0904: A New Polar at the Lower Period Limit

Author(s):  
V. Burwitz ◽  
K. Reinsch ◽  
A. D. Schwope ◽  
K. Beuermann ◽  
S. Mengel ◽  
...  
Keyword(s):  
1996 ◽  
Vol 158 ◽  
pp. 229-230
Author(s):  
V. Burwitz ◽  
K. Reinsch ◽  
A. D. Schwope ◽  
K. Beuermann ◽  
S. Mengel ◽  
...  

AbstractWe present X-ray and optical observations of the ROSAT discovered polar (AM Her binary) RX J1015.5+0904 and first results of our analysis of the X-ray and optical data. These results indicate a one-pole accretion geometry and an orbital period of P = 79.88 m for this V ~ 17 mag system.


Metrology ◽  
2022 ◽  
Vol 2 (1) ◽  
pp. 19-32
Author(s):  
Janik Schaude ◽  
Andreas Christian Gröschl ◽  
Tino Hausotte

The article presents the determination of the topographic spatial resolution of an optical point sensor. It is quantified by the lateral period limit DLIM measured on a type ASG material measure, also called (topographic) Siemens star, with a confocal sensor following both a radial measurement and evaluation, as proposed by ISO 25178-70, and the measurement and subsequent evaluation of two line scans, proposed by the NPL Good Practice Guide. As will be shown, for the latter, an only slightly misidentified target centre of the Siemens star leads to quite significant errors of the determined DLIM. Remarkably, a misidentified target centre does not necessarily result in an overestimation of DLIM, but lower values might also be obtained. Therefore, a modified Good Practice Guide is proposed to determine DLIM more accurately, as it includes a thorough determination of the centre of the Siemens star as well. While the measurement and evaluation effort is increased slightly compared to the NPL Good Practice Guide, it is still much faster than a complete radial measurement and evaluation.


2015 ◽  
Vol 2 (1) ◽  
pp. 41-45
Author(s):  
S. Zharikov ◽  
G. Tovmassian

We discussed features of Cataclysmic Variables at the period minimum. In general, most of them must be WZ Sge-type objects. Main characteristics of the prototype star (WZ Sge) are discussed. A part of WZ Sge-type objects has evolved past the period limit and formed the bounce back systems. We also explore conditions and structure of accretion disks in such systems. We show that the accretion disk in a system with extreme mass ratio grows in size reaching a 2:1 resonance radius and are relatively cool. They also become largely optically thin in the continuum, contributing to the total flux less than the stellar components of the system. In contrast, the viscosity and the temperature in spiral arms formed at the outer edge of the disk are higher and their contribution in continuum plays an increasingly important role. We model such disks and generate light curves which successfully simulate the observed double-humped light curves in the quiescence.


2019 ◽  
Vol 492 (2) ◽  
pp. 2731-2738 ◽  
Author(s):  
Dengkai Jiang

ABSTRACT Close detached binaries were theoretically predicted to evolve into contact by three subtypes of case A binary evolution, cases AD, AR, and AS, which correspond to the formation of contact during dynamic-, thermal-, and nuclear-time-scale mass transfer phases, respectively. It is unclear, however, what is the difference between contact binaries in these subtypes, and whether all of these subtypes can account for the formation of observed W Ursae Majoris (W UMa) binaries. Using Eggleton’s stellar evolution code with the non-conservative assumption, I obtained the low-mass contact binaries produced by cases AD, AR, and AS at the moment of contact and their parameter spaces. The results support that the progenitors of low-mass contact binaries are detached binaries with orbital periods shorter than $\sim 2\!-\!5\,$ d, and their borderlines depend strongly on the primary mass. In addition, the period–colour relations for cases AR and AS can be in better agreement with that for observed W UMa candidates, but case AD shows a significantly worse agreement. Moreover, cases AR and AS can produce a short-period limit (corresponding to a low-mass limit) at almost any age, e.g. from young age ($\sim 0.2\,$ Gyr) to old age ($\sim 13\,$ Gyr), agreeing with observed W UMa binaries in star clusters, but no such limit occurs for case AD at any age. These results support that cases AR and AS, as opposed to case AD, can lead to W UMa binaries (including young W UMa binaries).


Music ◽  
2019 ◽  
Author(s):  
Luca Lévi Sala

Mutius Philippus Vincentius Franciscus Xaverius Clementi (b. 1752–d. 1832) was an Italian composer, a pianist virtuoso and conductor, a teacher, a publisher, and a musical entrepreneur. Son of Niccolò Clementi and Magdalena (née Kaiser), he was educated in Rome with, among others, Antonio Boroni and Gaetano Carpani. An oratorio (disp 1, old WO1), now lost, is dating from 1764. In 1766 he moved to Dorset (United Kingdom), following the English nobleman Peter Beckford (b. 1740–d. 1811), which assured him a solid continuity in the study of composition and the practice of the harpsichord. From around 1774 and 1780, Clementi settled in London, where he appeared in piano performances and composed his first works for piano, comprising solo and accompanied sonatas (Opp. 1–4 and the Op-sn 17, old WO2). Between 1780 and 1785, Clementi traveled for his first European trip between Paris, Lyons, and Vienna, where he appeared before the Emperor Joseph II for the famous piano competition with Mozart on 24 December 1781. During these years, Clementi composed the Opp. 5 and 6 (published in Paris by Bailleux) and the so-called “Viennese” sonatas Opp. 7–10 (published by Artaria, Castaud and Torricella), also comprising the Toccata Op. 11, the Op. 12, and other pieces. Back to London, Clementi continued his career as a performer (until around early 1790) and as a teacher. Belonging to this period is the largest part of Clementi’s musical production (from Op. 13 to Op. 39) made of solo and accompanied piano sonatas, the two symphonies Op. 18, also comprising his first musical tutor, the Introduction to the Art of Playing on the Piano Forte (Op. 42, 1801) and the Practical Harmony (Op-sn 38, old WO7, 1801–). Following the bankruptcy of Longman & Broderip, on 1 November 1798 Clementi became a senior partner in Longman, Clementi, and Co. and from 1801 onwards he founded Muzio Clementi & Co., establishing a successful business activity as a music publisher, as a piano maker and a music dealer for around thirty years. He started business relationships with Pleyel in Paris, Breitkopf and Härtel in Leipzig and Artaria in Vienna, reaching important goals as the contract with Haydn and the one with Beethoven of 1807. From the summer 1802 until 1810, Clementi traveled to the continental Europe, dealing mainly with the sponsoring of his business firm. His compositions for this period limit to Opp. 40 and 41, the Op-sn 12, old WO8, the Op. 50 (though published later in 1821), plenty of arrangements for piano and a huge number of revisions aimed at the inclusion within Breitkopf & Härtel’s important project of the Œuvres Complettes (1803–1819) and for his own firm. In the last period of his life, Clementi focused on the composition of his four major symphonies (remained unpublished), the Appendix Op. 43, the three volumes of the Gradus ad Parnassum Op. 44 (1817–1826), and the Opp. 46–49, the Opp-sn 25, 1 and 2 (old WO9, WO10, and WO11). Beyond being published by Clementi’s own publishing firms, Clementi’s works and revisions were reissued extensively by Welcker, Preston, Dale, Longman & Broderip, Bailleux, Sieber, Imbault, Porro, Castaud, Artaria, André, Breitkopf & Härtel, and Hoffmeister.


1994 ◽  
Vol 04 (03) ◽  
pp. 609-621
Author(s):  
Lj. KOCAREV ◽  
Z. TASEV ◽  
D. DIMOVSKI ◽  
L.O. CHUA

Induced templates for two members of Chua’s attractors: spiral-type and double-scroll chaotic attractors are computed using the orbits of lower period. The template describes the topological properties of periodic orbits embedded in the attractor. It is identified by a set of integers which characterize the attractor. The templates are confirmed by investigating orbits of higher period.


New Astronomy ◽  
2017 ◽  
Vol 54 ◽  
pp. 52-55 ◽  
Author(s):  
Zhang Bin ◽  
Qian Shengbang ◽  
Miloslav Zejda ◽  
Zhu Liying ◽  
Liu Nianping

2020 ◽  
Vol 56 (2) ◽  
pp. 225-234
Author(s):  
M. Martignoni ◽  
C. Barani ◽  
F. Acerbi ◽  
R. Michel

The multicolour CCD light curves of the eclipsing binary systems CRTS J213033.6+213159 and 1SWASP J212454.61+203030.8 are presented for the first time, the observations are analyzed using the latest version of the WilsonDevinney code. Both the systems are found to be W UMa contact binaries belonging two different subtypes. All the light curves show the inverse O'Connell effect. By using our 2 times of minimum light for both the systems and the 187 and 105 ToMs extract from the SWASP observations, respectively for CRTS J213033.6+213159 and for 1SWASP J212454.61+203030.8, the orbital periods are here revised. The spectral type K of the systems and their short orbital periods (< 0.3 days), suggests that they are near the shortest period limit. The absolute dimensions are estimated and, from statistical diagrams, it is found that both components of the systems follow the general pattern of the relative subtype of W Ursae Majoris systems.


2007 ◽  
Vol 93 (1) ◽  
pp. 12-16
Author(s):  
G L Micheal ◽  
N. T. Fear ◽  
J. Hacker Hughes

AbstractObjectivesTo examine the pattern of out-patient mental health care referrals for military personnel deployed to the Falklands Islands, 1986-96.MethodsData from referral books of British Military Community Mental Health Nurses based in the Falkland Islands were abstracted, entered into an electronic database and analysed.ResultsOver the period 1986-96, 538 Service personnel were referred to the mental health out-patient facility on the Falkland Islands. The majority were male (96%) and junior ranks (81%). Approximately a third of patients were referred for reasons relating to alcohol (31%) and for over two-thirds of patients no follow-up was required (68%). Differences were observed by Service with the Army having more referrals due to alcohol than the other two Services, whilst the Navy had more deliberate self-harm referrals and the RAF more referrals for anxiety.ConclusionsThe lack of information on the total population deployed to the Falkland Islands over this period limit the interpretation of the results.


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