Palomar Testbed Interferometer Observations of Young Stellar Objects     

F.P. Wilkin  R.L. Akeson 《Astrophysics and Space Science》2003,286(1-2):145-150

We present observations of a sample of Herbig AeBe stars, as well as the FU Orionis object V1057 Cygni. Our K-band (2.2μm) observations from the Palomar Testbed Interferometer (PTI) used baselines of 110 m and 85 m, resulting in fringe spacings of ∼4 mas and 5 mas, respectively. Fringes were obtained for the first time on V1057 Cygnias well as V594 Cas. Additional measurements were made of MWC147, while upper limits to visibility-squared are obtained for MWC297, HD190073, and MWC614. These measurements are sensitive to the distribution of warm, circumstellar dust in these sources. If the circumstellar infrared emission comes from warm dust in a disk, the inclination of the disk to the line of sight implies that the observed interferometric visibilities should depend upon hour angle. Surprisingly, the observations of Millan-Gabet, Schloerb and Traub (2001)(hereafter MST) did not show significant variation with hour angle. However, limited sampling of angular frequencies on the sky was possible with the IOTA interferometer, motivating us to study a subset of their objects to further constrain these systems. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

单体褶牡蛎(Crassostrea sp.)的研究     

王昭萍  王如才  徐从先  仇宝志  姜福正  张祝绪 《中国海洋大学学报(自然科学版)》1992,(2)

采用肾上腺素(EPI)和去甲肾上腺素(NE)诱导、颗粒固着基和先固着后脱基三种方法,对褶牡蛎的眼点幼虫进行处理,产生单体蛎苗。EPI和NE诱导的最适浓度为10~(-4)M,最适处理时间为3h,幼虫的不固着变态率分别达47.7％和46.6％。处理时间延长,变态率增加不明显。EPI和NE的诱导效果差别不明显,其诱导作用对稚贝的生长无明显副作用。颗粒固着基以贝壳粉为佳,最适颗粒的规格为幼虫的壳长。幼虫先固着后脱基而形成单体蛎苗,以可弯曲的灰色塑料板效果最好,固着的小贝可通过来回弯曲塑料板而从上面脱落下来,小贝长至1～2cm大小时,脱基最容易。  相似文献   

A preliminary estimate of how stream water age is influenced by changing runoff sources in the Nagqu river water shed,Qinghai-Tibet Plateau     

Yuheng Yang  Baisha Weng  Denghua Yan  Xiaoyan Gong  Yanyu Dai  Yongzhen Niu 《水文研究》2021,35(10):e14380

  相似文献   

Detection of optical circular polarization in the Herbig Ae star WW Vul     

D. N. Shakhovskoi  O. S. Shulov  E. N. Kopatskaya 《Astronomy Letters》2001,27(6):376-378

UBVRI observations of circular polarization in WW Vul are presented. A positive polarization of ～0.1% was detected with a signal-to-noise ratio from 3 to 5 in each of the bands and more than 5 when averaged over all five bands. This observed polarization roughly corresponds to a 1% circular polarization of the radiation scattered in a circumstellar disk, which is most likely attributable to the significant alignment of scattering nonspherical dust grains. Since grain alignment is possible only in a magnetic field, this result provides circumstantial evidence for the existence of a magnetic field in the circumstellar disk of WW Vul.  相似文献   

天体物理环境中的硅酸盐尘粒   总被引：1，自引：0，他引：1  

李墨萍  赵刚  李爱根 《天文学进展》2007,25(2):132-146

硅酸盐尘粒是宇宙尘埃的主要成分之一,它广泛存在于许多天体物理环境中,其特性随环境而变化。由于近年来观测数据的不断增加和红外光谱质量的逐步提高,宇宙空间中的硅酸盐尘粒正受到越来越多的关注．该文详细地介绍了在各种天体环境(星际空间、演化晚期恒星的星周尘埃包层、绕年轻恒星和主序星的星周尘埃盘、彗星的彗发和行星际空间)中的硅酸盐尘粒的观测特征,并分别对其物理和化学性质进行了综合比较．观测已经证实在星际尘埃演化的前身(演化晚期恒星的星周尘埃包层)和其遗迹(彗星)均有可观数量的结晶硅酸盐存在。但是至今还没有在其中间态(弥散星际介质)找到结晶硅酸盐存在的证据。这一尚未解决的难题突出了结晶态硅酸盐在天体物理研究中的重要意义。  相似文献   

原行星盘的研究进展     

刘尧  王红池 《天文学进展》2011,29(2):148-167

原行星盘是环绕在年轻星天体(如T Tauri型星,HAe/Be星)周围的气体尘埃盘,是具有初始角动量的分子云核在塌缩形成恒星过程中的自然结果,是行星系统的起源地。原行星盘研究不仅是恒星形成理论的重要组成部分,而且是行星形成理论的基础。首先介绍了盘的形成与演化规律;然后介绍了年轻星天体的能谱分布,盘的模型和参数(质量吸积率、质量、尺度、温度、寿命);随后讨论了尘埃颗粒在盘中生长的观测证据以及行星在盘中形成的大致过程;最后对原行星盘研究的现状和未来做了总结与展望。  相似文献   

Hydrodynamic processes in young binaries as a source of cyclic variations in circumstellar extinction     

N. Ya. Sotnikova  V. P. Grinin 《Astronomy Letters》2007,33(9):594-603

Hydrodynamic models of a young binary accreting matter from the remnants of a protostellar cloud have been calculated by the SPH method. Periodic variations in column density in projection onto the primary component are shown to take place at low inclinations of the binary plane to the line of sight. These can result in periodic extinction variations accompanied by brightness variations in the primary. Generally, there can be three periodic components. The first component has a period equal to the orbital one and is attributable to the streams of matter penetrating into the inner regions of the binary. The second component has a period that is a factor of 5–8 longer than the orbital one and is related to the density waves generated in a circumbinary (CB) disk. Finally, the third, longest period is attributable to the precession of the inner CB disk regions. The relationship between the amplitudes of these cycles depends on the model parameters as well as on the inclination and orientation of the binary in space. We show that at a dust-togas ratio of 1: 100 and amass extinction coefficient of 250 cm² g^?1, the amplitude of the V-band brightness variations in the primary component can reach 1 ^m at a mass accretion rate onto the binary components of 10.8^?8 M _⊙ yr^?1 and a 10° inclination of the binary plane to the line of sight. We discuss possible applications of the model to young, pre-main-sequence stars.  相似文献   

摄食水平和温度对军曹鱼幼鱼生长及氮收支的影响          下载免费PDF全文

孙丽华  陈浩如 《热带海洋学报》2014,33(2):37-44

研究了不同摄食水平(从饥饿至饱食)和温度(21℃、27℃和33℃)对军曹鱼幼鱼(平均初始体重约10g)生长和氮收支的影响,并建立了生长-摄食/温度关系和不同摄食水平和温度条件下的氮收支方程。结果表明,在实验的温度范围内,军曹鱼幼鱼特定生长率均随摄食水平的增加呈显著增长趋势,生长-摄食关系在33℃时表现为线性相关,在27℃和21℃时表现为减速增长趋势,采用对数函数定量描述;在实验的摄食范围内(饥饿组除外),军曹鱼特定生长率随温度增加呈增长或先升后降的变化趋势,两者间的关系均采用二次函数定量描述。在实验的温度范围内,随摄食水平增加,军曹鱼幼鱼食物转化效率在水温33℃和21℃时呈增长趋势,在水温27℃时呈先升后降的变化趋势;在实验的摄食范围内(饥饿组除外),军曹鱼幼鱼食物转化效率随温度增加呈增长或先升后降的变化趋势,饱食时虽然食物转化效率最大值出现在33℃时,但方差分析显示33℃和27℃之间无显著性差异,其他摄食水平组在27℃时有最大值。在实验的摄食水平和温度范围内,军曹鱼幼鱼的排泄氮随摄食水平和温度的增加均呈显著增长趋势。  相似文献   

年轻造山带洋板块地层^*          下载免费PDF全文

马慧磊  许淑梅  李三忠  舒鹏程  崔慧琪  孔家豪 《古地理学报》2022,24(1):11-32

重点分析和总结了由显生宙增生复合体和造山带混杂岩重建的年轻造山带洋板块地层--太平洋洋板块地层,也简要介绍了东古印度洋(东新特提斯洋)和古亚洲洋洋板块地层的重建情况。通过对阿拉斯加南部中生代增生地体、俄罗斯远东和中国东北侏罗纪-早白垩世增生复合体、日本二叠纪-侏罗纪-白垩纪等不同时期的增生复合体、菲律宾侏罗纪增生复合体和美国加州海岸山脉中侏罗世-古新世弗朗西斯卡杂岩体等不同单元的岩石学特征、古生物地层学、年代地层学、因逆冲导致的构造叠置和混杂失序特征及演化阶段的分析,重建了太平洋洋板块地层。其中加州海岸山脉中侏罗世-古新世弗朗西斯卡杂岩体的研究比较深入,对该区俯冲带上叠蛇绿岩(大峡谷群弧前盆地蛇绿岩)和弗朗西斯卡北部马林海岬杂岩体(原岩为洋中脊玄武岩)进行了有效区分,不仅还原了太平洋板块的俯冲碰撞过程,还厘清了与之伴生的弧前盆地裂陷和扩张过程。另外,板块俯冲的滞留和幕式增生在活动时间较短的板块俯冲体系中可能不容易识别。  相似文献   

追忆五四运动中的地质青年     

焦奇 《地质论评》2022,68(5):1997-2002

通过分析五四运动的相关研究成果和研究部分地质青年的史料,介绍地质青年在五四运动中的作为,展现地质青年爱国报国的风貌,提出新时代地质青年应不忘历史,学习习总书记有关青年的讲话精神,在新时代的地质工作中弘扬五四精神和地质先辈精神,融入地质工作实践,推进地质事业转型发展。  相似文献