scholarly journals The puzzle of combination frequencies found in heat-driven pulsators

2012 ◽  
Vol 333 (10) ◽  
pp. 1053-1056 ◽  
Author(s):  
P.I. Pápics
1987 ◽  
Vol 30 (2) ◽  
pp. 189-206 ◽  
Author(s):  
P. P. Belyaev ◽  
D. S. Kotik ◽  
S. N. Mityakov ◽  
S. V. Polyakov ◽  
V. O. Rapoport ◽  
...  

2019 ◽  
Vol 13 (5-6) ◽  
pp. 221-227
Author(s):  
Mona K. Mekkawy ◽  
Alaa K. Kamel ◽  
Nabil Dessouky ◽  
Mohamed Elgharbawy ◽  
Inas Mazen

Ovotesticular difference of sex development (OT DSD) is a rare genetic disorder with an incidence of about 1/100,000 live births. The majority of OT DSD patients show a 46,XX karyotype, others may have 46,XX/46,XY chimerism or exhibit various mosaic sex chromosome combinations, and less commonly they may have a 46,XY karyotype. The aim of this work is to report the clinical, pathological, and karyotypic variations in OT DSD patients diagnosed among a large cohort of DSD patients. The study included 10 patients thoroughly evaluated for clinical, genital, and hormonal abnormalities and subjected to imaging studies, laparoscopy with gonadal biopsy, karyotype, and FISH analysis. The current study revealed a greater percentage of mosaic cell line combinations than previously reported and showed variable cytogenetic abnormalities, including the rare isodicentric (Y)(p11.32) abnormality and X;Y translocation. The study also revealed a unique pattern of gonadal type and combination frequencies. To our knowledge, this is the first study on OT DSD patients among a large cohort of DSD patients in Egypt and the Middle East.


2018 ◽  
Vol 620 ◽  
pp. A145 ◽  
Author(s):  
D. Baade ◽  
A. Pigulski ◽  
Th. Rivinius ◽  
L. Wang ◽  
Ch. Martayan ◽  
...  

Context. In early-type Be stars, groups of nonradial pulsation (NRP) modes with numerically related frequencies may be instrumental for the release of excess angular momentum through mass-ejection events. Difference and sum/harmonic frequencies often form additional groups. Aims. The purpose of this study is to find out whether a similar frequency pattern occurs in the cooler third-magnitude B7-8 IIIe shell star ν Pup. Methods. Time-series analyses were performed of space photometry with BRITE-Constellation (2015, 2016/17, and 2017/18), SMEI (2003–2011), and HIPPARCOS (1989–1993). Two IUE SWP and 27 optical echelle spectra spanning 20 years were retrieved from various archives. Results. The optical spectra exhibit no anomalies or well-defined variabilities. A magnetic field was not detected. All three photometry satellites recorded variability near 0.656 c/d which is resolved into three features separated by ∼0.0021 c/d. Their first harmonics and two combination frequencies form a second group, whose features are similarly spaced by 0.0021 c/d. The frequency spacing is very nearly but not exactly equidistant. Variability near 0.0021 c/d was not detected. The long-term frequency stability could be used to derive meaningful constraints on the properties of a putative companion star. The IUE spectra do not reveal the presence of a hot subluminous secondary. Conclusions. ν Pup is another Be star exhibiting an NRP variability pattern with long-term constancy and underlining the importance of combination frequencies and frequency groups. This star is a good target for efforts to identify an effectively single Be star.


1995 ◽  
Vol 155 ◽  
pp. 331-332
Author(s):  
G. Handler ◽  
D. O’Donoghue ◽  
D. A. H. Buckley ◽  
O. Giovannini ◽  
S. O. Kepler ◽  
...  

The variability of CD-24 7599 (V=11.48 mag) was discovered by JCC during observing run XCOV7 of the Whole Earth Telescope (WET, Nather et al. 1990) network in February, 1992. The star was observed as an additional target and 117 hours of high-quality temporal spectroscopic observations were obtained.Our analysis of these data revealed the presence of 7 independent pulsation modes between 27.0 and 38.1 cycles per day (313 – 441 μHz) with semiamplitudes of 2.1 – 10.2 milli-modulation amplitudes (mma). We showed that peaks at linear combination frequencies detected in the power spectra were not due to eigenmodes excited to visible amplitude by resonant mode coupling.


Author(s):  
Jerzy T. Sawicki ◽  
Dmitry L. Storozhev ◽  
John D. Lekki

This paper addresses self-diagnostic properties of AMB (active magnetic bearing) supported rotors for on-line detection of the transverse crack on a rotating shaft. In addition to pure levitation, the rotor supporting bearing also serves as an actuator that transforms current signals additionally injected into the control loop into the superimposed specially selected excitation forces into the suspended rotor. These additional excitations induce combination frequencies in the rotor response, providing unique signatures for the presence of crack. The background of theoretical modeling, experimental and computer simulation results for the AMB supported cracked rotor with self-diagnostic excitation forces are presented and discussed.


1979 ◽  
Vol 32 (3) ◽  
pp. 481 ◽  
Author(s):  
E Spinner ◽  
JE Rowe

Infrared spectra (4000-200 cm-1; KBr discs) have been obtained for ten isotopic species of solid sodium formate in bulk (isotopic purities ranging from 80% to 99%) and after isotopic dilution. In probably the most systematic and comprehensive study of its kind to date on a polyatomic solid, a large number of solid solutions, such as H12C16O2Na in D13C18O2Na and vice versa, D12C16O2Na in D13C18O2Na and vice versa, etc., have been examined (solute concentration usually in the range from 15% to 1 %). The CH and CD out-of-plane and in-plane bending frequencies are raised somewhat on isotopic dilution, the CH and CD stretching, OCO scissoring and lower CO stretching frequencies are lowered a little. For the latter two vibrations the frequency of the solid solute is affected by that of the solid solvent only very slightly (by 0.5 cm-1 to 1.0 cm-1), but in a very regular and systematic manner. For the higher carboxylate stretching frequency, by contrast, the effect of isotopic dilution is much more varied. The solute frequency is raised (e.g. by 3.5 cm-1 for H12C16O2Na in D13C18O2Na), or lowered (e.g. by 6.5 cm-1 for D13C18O2Na in H12C16O2Na, 18 cm-1 for H13C16O2Na in H12C16O2Na, 22 cm-1 for H13C16O2Na in D13C18O2Na), depending on whether the intrinsic solute frequency is higher or lower than that of the solvent, and by an amount determined by the separation between the two. Thus, for this vibration strong coupling between solute anion and solvent anions is still conspicuous after isotopic dilution, and the 'solute' spectra observed are those of a cluster of solute anion surrounded by solvent anions; they do not usually approximate to the spectra of individual isolated solute ions. Some combination frequencies show much lower anharmonicity corrections after isotopic dilution than in bulk. With isotopically mixed crystals transfer of absorption intensity is observed, to the bands at lower frequencies for CH and CD in- and out-of-plane bending, and to those at higher frequencies for OCO scissoring and both CO stretching vibrations. For larger crystals and solid films, an instance was found of a large intensity transfer to higher frequencies, additional to the (small) one seen with KBr discs. A satisfactory explanation in terms of the crystal structure is at present available only for the out- of-plane bending results.


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