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Arthur Lei Qiu

Publications and source records attributed to Arthur Lei Qiu.

2 recordsLinked to original sources

Weighted linearization of vector fields via a formal Moser trick

Many well-known theorems establish sufficient criteria for linearizability of a vector field in terms of the eigenvalues of its linear approximation. By attaching weights to coordinates so that some directions are considered "linear", others "quadratic", and so on, one can define the notion of a weighted linear approximation. It is thus natural to ask when a vector field is "weighted-linearizable". In this paper, we formulate a weighted version of the non-resonance condition appearing in the Poincaré and Sternberg linearization theorems and show that it implies weighted linearizability. Our approach first addresses weighted linearization on the level of formal power series. In doing so, we develop a general framework to make sense of a power series version of Moser's trick, a technique used to prove various normal form results in geometry. This formal Moser trick works over any field of characteristic zero and may be of independent interest.

math.DG

Long-Term Changes in the Variability of Pulsating Red Giants (and One R CrB Star)

We have used many decades of visual observations from the AAVSO International Database, and the AAVSO time-series analysis package VSTAR, to study the long-term changes in period, amplitude, and mean magnitude in about 30 normal pulsating red giants (PRGs) i.e. those without large secular changes in period, as well as a few of the rare PRGs which do have such secular period changes. The periods of the typical PRGs "wander" on time scales of about 40 pulsation periods -- significantly longer than the time scales of amplitude variation which are 20-35 with a mean of 27 pulsation periods. We have also studied the range and time scale of the long-term changes in pulsation amplitude and mean magnitude, as well as period, and looked for correlations between these. Changes in mean magnitude are larger in stars in stars with larger mean amplitude, but correlate negatively with changes in amplitude. There is a weak positive correlation between the long-term period changes and amplitude changes. The causes of these three kinds of long-term changes are still not clear. We note, from the presence of harmonics in the Fourier spectra, that the longest-period PRGs have distinctly non-sinusoidal phase curves. For studying PRGs, we demonstrate the advantage of studying stars with minimal seasonal gaps in the observations, such as those near the celestial poles. We studied Z UMi, misclassified as a possible Mira star, but actually an R CrB star. We determined times of onset of 16 fadings. We were not able to determine a coherent pulsation period for this star at maximum, with an amplitude greater than 0.05. We did, however, find that the times of onset of fadings were "locked" to a 41.98-day period -- a typical pulsation period for an R CrB star.

astro-ph.SR