Porous metallic material has become a kind of typical multifunctional material with the quick development of advanced manufacturing and forming process technologies in past years. At present, it has also been a structural function material with the characteristics of ultra-light weight, high specific strength and rigidity. As a sound absorbing material in noise control engineering, the acoustic...

We adapt the method of Simon [26] to prove a $C^{1,\alpha}$-regularity theorem for minimal varifolds which resemble cone $\mathbf{C}^2_0$ over an equiangular geodesic net. For varifold classes admitting “no-hole” condition on singular set, we additionally establish near $\mathbf{C}^2_0 \times \mathbb{R}^m$. Combined with work Allard [2], [26], Taylor [29], and Naber–Valtorta [21], our result im...

Ten species of the genus Aulacophora Chevrolat, 1836 are reported for Taiwan. Specimens of A. opacipennis Chûjô, 1962 collected from Southeast Asia were misidentified by Kimoto (1989) and should be identified as A. apicipes Jacoby, 1896. Color photos of habitus and drawings of male and female genitalia from eleven species (including A. apicipes) are presented. The following synonymies are propo...

We make use of the Next Generation model atmospheres by Allard et al. (1997) and Hauschildt, Allard & Baron (1999) to compute theoretical models for low and very low-mass stars for selected metallicities in the range Z= 0.0002 to 0.002. On this basis, we present theoretical predictions covering the sequence of H-burning stars as observed in galactic globulars from the faint end of the Main Sequ...

In this autoethnographic critical self-inquiry study, I draw upon my unique identity as once a Chinese international student and now an English professor at private research university in the United States to investigate how sought for multilingual empowered students while coping with linguicism monolingual ideologies. Despite increasing cultural linguistic diversity population, faculty body de...

We present a spectroscopic classification system for M-dwarfs and M-subdwarfs based on quantitative measures of TiO and CaH features in the region λλ6200−7400Å. Our sample of cool stars covers the range from solar metallicity stars to the most extreme subdwarfs known. Using synthetic spectra computed by Allard and Hauschildt (1995), we derive metallicities for the stars. Stars are classified as...

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