Age and Mass Estimates for 41 Star Clusters in M33

In this second paper of our series, we estimate the age of 41 star clusters, which were detected by Melnick & D'odorico in the nearby spiral galaxy M33, by comparing the integrated photometric measurements with theoretical stellar population synthesis models of Bruzual & Charlot. Also, we calculate the mass of these star clusters using the theoretical M/LV ratio. The results show that, these star clusters formed continuously in M33 from ~ 7 × 106–1010 years and have masses between ~ 103 and 2 × 106M☉. M33 frames were observed as a part of the BATC Multicolor Survey of the sky in 13 intermediate-band filters from 3800 to 10 000?. The relation between age and mass confirms that the sample star cluster masses systematically decrease from the oldest to the youngest.

Positions and Spectral Energy Distributions of 41 Star Clusters in M33

We present accurate positions and multi-color photometry for 41 star clusters detected by Melnick & D'odorico in the nearby spiral galaxy M33 as a part of the BATC Color Survey of the sky in 13 intermediate-band filters from 3800 to 10 000 A. The coordinates of the clusters are found from the HST Guide Star Catalog. By aperture photometry, we obtain the spectral energy distributions of the clusters. Using the relations between the BATC intermediate-band system and UBVRI broadband system, we derive their V magnitudes and B - V colors and find that most of them are blue, which is consistent with previous findings.

M33的化学演化研究

作为本星系群中的旋涡星系之一,M33(NGC 598)是验证星系化学演化理论不可多得的目标,因为它具有适当的距离和角直径,使得现今对其气体、恒星形成率(SFR)及丰度进行精细观测成为可能。该文首先对:M33的盘建立了化学演化模型,同时考虑了内落和外流的影响,详细讨论了吸积和坍缩两种盘的内落模型。由于M33的质量较小、势阱较浅,容易受超新星爆发等过程的影响而引发外流,因此除了讨论内落时标的影响外,文中还讨论了与SFR成正比的外流的作用。得到了3条主要结论:(1)无论是坍缩模型还是吸积模型,在内落时标较长的时候,都可以给出较满意的结果,说明M33是通过慢速吸积过程形成的;(2)通过对M33的金属丰度研究表明,外流必不可少;(3)在采用较长的内落时标和引入外流后,与银河系相似的修正K-S定律可以较好地重现各个观测约束。

C_0-Semigroup Method of the Density Evolution Equation for M/M/∞ Model

In this paper, the existence, uniqueness, and asymptotic behavior of the solution of the density evolution equation for M/M/∞ model was studied by the semigroup theory of linear operators.

Estimating the Metallicity of Old Star Clusters in M33

Based on the method proposed by Kong et al. and on the multi-color spectrophotometry by Ma et al., we estimate the metallicities of 16 old star clusters in the nearby spiral galaxy M33, ten of which are halo globular clusters. These old clusters are all metal poor, the range of metallicity ([Fe/H]) is from-0.14 to-2.12. In general, our results are consistent with those derived by other methods, such as integrated spectra and photometry, and our study confirms the reliability of the method of Kong et al.

The LAMOST survey of background quasars in the vicinity of M31 and M33–Ⅲ.results from the 2013 regular survey

In this work, we report new quasars discovered in fields in the vicinity of the Andromeda（M31） and Triangulum（M33） galaxies with the Large Sky Area Multi-Object Fiber Spectroscopic Telescope（LAMOST, also called the Guo Shou Jing Telescope） during the 2013 observational season, the second year of the regular survey. In total, 1330 new quasars are discovered in an area of ～133 deg2 around M31and M33. With i magnitudes ranging from 14.79 to 20.0 and redshifts from 0.08 to4.85, the 1330 new quasars represent a significant increase in the number of identified quasars in fields in the vicinity of M31 and M33. Up to now, there have been a total of 1870 quasars discovered by LAMOST in this area. The much enlarged sample of known quasars in this area can potentially be utilized to construct a precise astrometric reference frame for the measurement of minute proper motions of M31, M33 and their associated substructures, which are vital for understanding the formation and evolution of M31, M33 and the Local Group of galaxies. Moreover, in the sample,there are a total of 45, 98 and 225 quasars with i magnitudes brighter than 17.0, 17.5and 18.0 respectively. In the aforementioned brightness bins, 15, 35 and 84 quasars are reported here for the first time, and 6, 21 and 81 are reported in our pervious work. In addition, 0, 1 and 6 are from the Sloan Digital Sky Survey and 24, 41 and 54 are from the NED database. These bright quasars provide an invaluable sample to study the kinematics and chemistry of the interstellar/intergalactic medium of the Local Group.

The LAMOST spectroscopic survey of globular clusters in M31and M33.I.catalog and new identifications

We present a catalog of 908 objects observed with the Large Sky Area Multi-Object Fiber Spectroscopic Telescope（LAMOST） in fields in the vicinity of M31 and M33, targeted as globular clusters（GCs） and candidates. The targets include known GCs and candidates selected from the literature, as well as new candidates selected from the Sloan Digital Sky Survey（SDSS）. Analysis shows that 356 of them are likely GCs with various confidence levels, while the remaining ones turn out to be background galaxies and quasars, stars and H II regions in M31 or foreground Galactic stars. The 356 likely GCs include 298 bona fide GCs and 26 candidates known in the literature. Three candidates, selected from the Revised Bologna Catalog of M31 GCs and candidates（RBC） and one possible cluster from Johnson et al., are confirmed to be bona fide clusters. We search for new GCs in the halo of the M31 among the new candidates selected from the SDSS photometry. Based on radial velocities yielded by LAMOST spectra and visual examination of the SDSS images, we find 28 objects, 5bona fide and 23 likely GCs. Among the five bona fide GCs, three have been recently discovered independently by others, and the remaining 25 are our new identifications,including two bona fide ones. The newly identified objects fall at projected distances ranging from 13 to 265 kpc from M31. Of the two newly discovered bona fide GCs,one is located near M33, probably a GC belonging to M33. The other bona fide GC falls on the Giant Stream with a projected distance of 78 kpc from M31. Of the 23 newly identified likely GCs, one has a projected distance of about 265 kpc from M31 and could be an intergalactic cluster.

PERTURBED NONLINEAR EVOLUTION INCLUSIONS IN BANACH SPACES

In this paper we discuss tLhe existence results of the integral solutions to nonlinear evolution inclusion: u' (t) ∈ Au(t) +F(t,u(t)), where A is m-dissipative and F is a set valued map in separable Banach spaces, and extend the relative results in references.

华硕台式电脑M33AAG 真材实料真品质

作为全球知名的IT企业,华硕始终视产品品质为安身立命之本,在每一个流程中时时强调品质管理与细节。经过上千项测试环节历练的产品品质,以及在品质管理和服务上的努力用心,展现出华硕磐石品质之根源,力求为所有用户提供世界级的产品和服务。华硕台式电脑M33AAG就是经过华硕严苛的品质测试,精心打造的一款台式电脑产品。卓越的外观设计打造好产品第一步华硕台式电脑M33AAG,拥有极为优秀的工业设计,机箱采用的27L大机体设计,机箱空间大幅度增加,更大的机身容量为机箱内提供了极好的散热空间。同时,采用1.0mm厚度板材,增强了机体的抗冲压能力,更为坚固可靠。在外观设计方面,机箱的前面板采用现代感十足的金属拉丝工艺,彰显时尚大气的设计风格;面板上部。

A catalogue of Hα emission-line point sources in the vicinity fields of M31 and M33 from the LAMOST survey

We present a catalogue of 3305 Hα emission-line point sources observed with the Large Sky Area Multi-Object Fiber Spectroscopic Telescope(LAMOST) in the vicinity fields of M31 and M33 during September 2011 and January 2016.The catalogue contains 1487 emission-line stars,532 emission-line nebulae including 377 likely planetary nebulae(PNe),83 H Ⅱ region candidates and 20 possible supernova remnants(SNRs) and 1286 unknown objects.Among them,24 PN candidates,19 H Ⅱ region candidates,10 SNR candidates and one symbiotic star candidate are new discoveries.Radial velocities and fluxes estimated from the Hα line and those quantities of seven other major emission lines including Hβ,[O Ⅲ] A4959,[O Ⅲ] A5007,[N Ⅱ] A6548,[N Ⅱ] A6583,[S Ⅱ] A6717 and [S Ⅱ] A6731 lines of all the catalogued sources yielded from the LAMOST spectra are also presented in our catalogue.Our catalogue is an ideal starting point to study the chemistry properties and kinematics of M 31 and M 33.

Temporal and Spatial Evolution of Precursory Anomalies of the Wenchuan MS8.0 Earthquake and Their Mechanical Analysis

In order to study the spatiotemporal evolution of the precursory anomalies 10 years before the Wenchuan M_S8. 0 earthquake in 2008, the epicentral distance of the precursory anomalies is calculated by using the geometric center of the rupture region and the elliptical centerline of the aftershock region. The result shows, precursor anomalies gradually increased about 2 years before the Wenchuan earthquake. The ratio of abnormal items is greater than 25% in the near source area (about twice the source scale) and 17%-24% in the remote area (about 3-5 times the source scale). There are three different stages of spatiotemporal evolution of precursory anomalies. During the α stage (including α_1 and α_2,between 700 to 3000 days before the main earthquake),the anomalies are mainly distributed in the southwest and northwest area of the Wenchuan aftershocks area. It is shown that the precursors of the far source region and the near source area have the characteristics of outward expansion. During the β stage (between 300 to 700 days before the main earthquake), the anomalies are distributed in the southwest and northern region of the aftershock region, showing a large range of anomalies. During the γ stage (including γ_1 and γ_2, 300 days before the main earthquake),the range of anomaly distribution is wide,and the anomalies are distributed in the southwest and northeast of the aftershock area. The anomalies converged to epicenter (γ_1) in the far source region and expand outwards (γ_2) in the near source region. Results of the experimental study and mechanical analysis of earthquake preparation process indicate that the three-stage characteristics of precursory anomalies in the process of earthquake preparation may be controlled by the seismogenic body,which is a form of expression in the process of earthquake preparation and a universal featureduring the earthquake preparation process,which has a certain guiding role in earthquake prediction.

河南义马上石河墓地M23、M33发掘简报

2018年4~8月,为配合义马市基本建设工程,河南省文物考古研究院等单位联合对位于义马市区南部的上石河墓地进行了抢救性考古发掘,清理了一批春秋时期墓葬。其中M23、M33属于春秋早期小型贵族墓葬,共出土各类器物241件(枚),质地有铜、玉、石、陶、骨等,为研究豫西地区春秋时期的葬制和葬俗提供了珍贵的考古材料。

Systematic analysis of distinct flow characteristics and underlying microstructural evolution mechanisms of a novel fine-grained P/M nickel-based superalloy during isothermal compression

Isothermal forging(IF)is an effective method for forming difficult-to-deform materials like P/M superalloys.Understanding the isothermal compression microstructural evolution mechanism of a novel P/M s-peralloy provides the basis for its optimized IF planning.In this study,the isothermal compression tests of a novel fine-grained P/M nickel-based superalloy were carried out at 1000-1150℃with strain rates of 0.001-0.01 s^(−1).The results indicated that the alloy exhibits three distinct flow characteristics:continuous softening after reaching the peak stress,near-steady superplastic flow,and discontinuous hardening,corresponding to different strain rate sensitivity exponent(m)values.Varied microstructural evolution mechanisms,including grain boundary sliding(GBS),dynamic recrystallization(DRX),and grain growth,are dominated in different m-value domains.Meanwhile,different roles of primaryγ’play in microstruc-tural evolution were clarified.A moderate fraction of primaryγ’with 8.5%-14.2%can well coordinate the GBS and hinder excessive grain growth at a high m value domain(m>0.4).When 0.2<m<0.4,the role of the primaryγ’is changed to promote dislocation accumulation,accelerating the nucleation of DRXed grains.As the primaryγ’is dissolved at 1150℃,obvious grain growth was observed after compression.Work hardening effect by overgrown grains competed with DRX softening results in the discontinuous rising stress.

论罗家坝M33的墓葬形制及文化属性

宣汉罗家坝巴文化墓地中规格最高的墓葬M33,实际上是两座具有打破关系的墓葬,被打破者为船棺合葬墓,出土器物受到了楚文化和蜀文化的影响,墓主人有可能属于巴文化的王者或高级贵族。

广州话禁止词“咪”为“唔使”合音证

“咪”是广州话中常见的表禁止或劝阻的否定副词。根据方言调查语料和方言历史文献,从音义两方面证明广州话禁止词“咪”确实是来自否定结构“唔使”的合音。合音形式“咪”原本和否定结构“唔使”里的“使”一样读阴上调,今读阳上调是根据合音形式的声母为次浊而作出的声调调整;历史上的“唔使”兼有必要性否定和禁止性否定两种用法,“唔使”合音为“咪”是在禁止祈使句中实现的,合音词“咪”继承的是“唔使”的禁止性否定用法。

制造业全球跨境并购网络空间格局演化及影响因素

本文以1997~2019年制造业全球跨境并购的交易事件数作为样本,探究2008年金融危机前后制造业跨境并购网络空间演变特征及其影响因素的差异性。结果发现:制造业跨境并购网络聚集程度略微降低,但网络联系的规模、强度及密度等均呈现增长的趋势;制造业跨境并购网络的重心由以欧美主导的经济体向亚太地区倾斜;推力因素包括经济、技术、自然资源和劳动力距离等资源标的动机均对制造业跨境并购联系的形成产生负向影响;拉力因素在金融危机前后对制造业跨境并购网络形成的影响不同;地理距离对其产生负向影响;而制度距离由2008年前的正向影响变为无影响;汇率和教育距离则分别由2008年前的无影响变为正向和负向影响。

基于STM32F103和M33的家居安防监视系统的硬件设计与实现

详细介绍了一种家居安防监视系统的硬件设计。该系统使用主控芯片STM32F103和模块M33,实现了图像采集和处理、GSM/GPRS通讯、短距离无线通讯、人机交互信息显示、红外感应、外部电源和内部锂电池供电等功能。实际运行表明,该系统具有可靠性好、功能强、成本低、安装和使用方便的特点,满足了人们对家居安防产品的要求。

宣汉罗家坝遗址M33的年代与墓主社会地位

宣汉罗家坝M33是一座典型的巴蜀文化墓葬,该墓包含了楚文化、中原文化、燕齐文化等多种外来文化铜器。在讨论了中赵甫墓、大黑汀M1、相家庄M6、辛店M2等相关典型墓葬年代的基础上,指出诸外来铜器年代最早者可到春秋晚期,最晚者为战国中期早段。在此基础上,结合巴蜀文化铜器和陶器的演变情况,可知该墓年代以战国中期早段(前395~前356年)为宜。从墓葬形制与规模、外来青铜器和土著青铜器的数量情况来看,墓主应为高级贵族。

并购情境下基于智力资本整合的技术追赶机理———沈阳机床并购德国希斯案例分析

跨国并购被认为是后发企业获取创新资源实现技术追赶的有效捷径。对被并方资源形式拥有并不等于技术能力提升,有效内化并购资源才能支持后发企业技术能力跃升。但文献对“并购-技术追赶”的资源整合的动态机制缺乏充分理论解释。将沈阳机床并购德国希斯的整合实践作为案例样本,借鉴与组织技术转移和创新关联性较强的“智力资本”概念体系,探索基于并购的“智力资本整合-技术追赶”内在机理。研究发现:①基于并购的技术追赶遵循“吸收模仿-集成创造-主导领先”发展路径;②“并购追赶”导向下智力资本整合呈现“人力资本整合主导-社会资本整合主导-组织资本整合主导”演进轨迹;③智力资本整合效应呈现“逆向吸收效应-多元融合效应-能力重构效应”动态转变。