旋涡星系随Hubble序列的一些统计性质     

马骏  赵君亮  张飞鹏  彭秋和 《天文学报》2000,41(2):172-180

对发表在Ａ＆ＡｐＳｕｐｐｌｅｍｅｎｔ Ｓｅｒｉｅｓ上３６５个旋涡星系的一些参数（如表示旋臂缠卷松紧程度的参数Λ、切向角ｕ、盘的扁度Ｈ／Ｄ２５以及厚度等）随Ｈｕｂｂｌｅ序列变化的关系进行了统计研究。首次得到这些参量的平均值;并且从统计结果可以明显地看到Ｈｕｂｂｌｅ对旋涡星系的分类只是一种定性的、只有统计意义上的分类;另外,从我们的统计结果看,密度波理论的色散关系对大多数旋涡星系是成立的,即大多数旋涡  相似文献   

Essential properties of the cD galaxy in Abell 1795 — II. Radio structure     

T. M. Kirchner  F. W. Baier  H. Tiersch 《Astronomische Nachrichten》1992,313(1):35-43

We consider current problems connected with the evolution of central dominant (cD) galaxies in clusters. In the second part of this series, internal properties of the cD galaxy — in particular its radio structure — are related to the appropriate ones of the cluster. The observations point to an earlier jet ejection along the major axis of the galaxy and a following change of the jet axis. From the existence of “hot-spot” like regions in different directions it is suggested that the radio engine would have to be intermittent with a relatively short period. Alternatively to the intermittent ejection scenario, the radio morphology of 4C 26.42 can be explained in the frame of the “standard” beam or jet model. The radio structure of 4C 26.42 being an inversion-symmetric configuration, which is probably due to galactic cannibalism, could be interpreted as a transition at the inner hot spots (at about 1 kpc) from supersonic, stable Fanaroff-Riley type II jets to subsonic, unstable FR I type structures (“plumes”). A quantitative investigation of the two scenarios for jet interaction with the surroudning interstellar/intercluster medium in 4C 26.42 gives parameter values in reasonable agreement with the ones discussed in the literature for related objects.  相似文献   

On the total kinetic energy of our galaxy     

S. Ninkovi&#x; 《Astronomische Nachrichten》1992,313(2):83-89

The total kinetic energy of the Galaxy is estimated from the potential energy by applying the virial theorem. The limits of the potential energy depend strongly on the value of the local escape velocity. They are estimated to be between −7. 10¹⁶ M_Ȯ km²s⁻² and −1. 10¹⁶ M_Ȯ km²s⁻² (escape velocity approximately between 450 km s⁻¹ and 600 km s⁻¹). The specific kinetic energy of the Galaxy as a whole is most likely about 21 000 km²s⁻², being equally distributed among the subsystems if the local escape velocity is near its lower limit; the higher the local escape velocity is, the higher is the specific kinetic energy of the Galaxy due to the influence of the dark corona. The specific kinetic energy of the dark corona tends to become equal to that of the Galaxy as a whole for very high values of the local escape velocity. For the purpose of estimating the totl potential energy of the Galaxy, inter alia, a new model of the Milky Way is developed, which yields both the potential and the density analytically so that it is suitale for calculating the galactocentric orbits.  相似文献   

Essential properties of the cD galaxy in Abell 1795 — I. General optical and X-ray structure,dynamics and formation     

F. W. Baier  T. M. Kirchner  H. Tiersch 《Astronomische Nachrichten》1992,313(1):21-33

We investigate current problems connected with the formation of cD galaxies. The subject of the present paper is to compare internal properties of the cD galaxy Zw162010 with cluster properties of Abell 1795. This consideration is a first attempt to find commonly valid essential correlations between peculiarities of brightest cluster members as structures and active phenomena and global cluster properties as for instance galaxy populations and concentration degrees. The colours, the X-ray emission, and the velocity of the cD galaxy are used to discuss the obvious influence of the environment on the evolution of the active nucleus. In a second paper (Kirchner et al. 1992) the radio structure is used to investigate the influence of the surrounding cluster medium onto the development of the active nucleus. Furtheron, various jet ejection scenarios will be quantitatively examined.  相似文献   

The irregular galaxy Cassiopeia 1 – a new member of the Local group     

N. Tikhonov 《Astronomische Nachrichten》1996,317(3):175-178

A photometry in the V, R, I (Cousins) system has been performed for stars in the galaxy Cassiopeia 1. The resulting colour-agnitude (CM) diagram of Cas 1 reveals the existence of blue stars and the absence of red ones. From an analysis of the CM diagram of the galaxy it is concluded that A_v = 4.0 mag, and the distance modulus (m – M)_o = 24.5 mag, corresponding to a distance of 790 kpc. The visual magnitude of the galaxy is V = 14^m.62 (M_v = −13^m.8) and the colour index (V – R) = 0.89 mag. From the distance determination the galaxy Cassiopeia 1 is a member of the Local group.  相似文献   

Photometric catalogue of Shakhbazian compact groups of galaxies. IV.     

D. Stoll  H. Tiersch  H. Oleak  H. T. Macgillivray 《Astronomische Nachrichten》1994,315(2):97-150

The fourth part of the photometric catalogue of Shakhbazian compact groups of galaxies contains optical and geometrical properties of another 26 groups (Shkh 313, 314, 315, 316, 317, 318, 319, 320, 321, 322, 323, 324, 325, 326, 327, 328, 329, 330, 331, 332, 333, 334, 335, 336, 337, 357). As in the previous papers photometric data were obtained from the COSMOS/UKST catalogue of the Southern sky with δ ± +2°30'. The survey of compact galaxy groups by Shakhbazian, Petrosian, Baier, and Tiersch is a basis for studying physical properties of such groups.  相似文献   

Investigation of the kinematics and structure of the Galaxy in the vicinity of the North galactic pole     

N. Kharchenko  E. Schilbach  R.-D. Scholz 《Astronomische Nachrichten》1994,315(4):291-301

In the framework of the programme of studying the meridional section of the Galaxy (MEGA) the absolute proper motions of more than 11000 stars with respect to 3000 galaxies and their stellar magnitudes in the B, V Johnson system are determined in two sky regions near the North Galactic Pole (NGP) by means of Tautenburg Schmidt plates. The limiting and completing apparent stellar magnitudes are B = 20.4 and 18.3 mag, the overall and the investigated sky areas are 16.4 and 14.6 square degrees, respectively. Distances have been determined using the stellar magnitudes, colours, proper motions and reduced proper motions. Stellar kinematics, eccentricities of Galactic orbits, spatial distribution and changes of these characteristics with Z-distance from the Galactic plane are obtained up to 15 kpc. Four subsystems distinguished in the NGP direction, respectively with semithicknesses of 0.25, 0.38, 0.67, 1.48 kpc and density ellipsoid axial ratios of 0.09, 0.20, 0.28, 0.49 show mean velocities in the Galactic rotation direction relative to the LSR of 5.6 ± 0.6, − 11.0 ± 0.6, − 62.5 ± 1.2, − 181.6 ± 4.4 km/s, and ages of 0.1, 0.4, 0.9, 1 of the Galaxy age.  相似文献   

池塘养殖脊尾白虾(Exopalaemon carinicauda)感染血卵涡鞭虫的研究   总被引：4，自引：2，他引：2  

许文军  谢建军  施慧  张静  张家松 《海洋与湖沼》2010,41(3):396-402

通过现场取样、显微镜检、细菌培养、组织病理、电镜观察以及PCR检测等研究手段,对2008年9月浙江省舟山市普陀区某梭子蟹养殖塘混养的脊尾白虾"白浊病"进行了系统的病原学研究。结果表明,病虾体色发白,反应迟钝,血淋巴液呈浊白色,严重患病白虾血淋巴中的血细胞几乎没有或者极少,代之以大量与血细胞形似的寄生虫;组织病理切片及电镜观察发现,病虾心脏、肝胰腺、肌肉、鳃部等组织寄生有大量单细胞寄生虫,该寄生虫虫体形态特征、显微结构及宿主临床症状与本实验室之前研究报道的感染三疣梭子蟹和锯缘青蟹的血卵涡鞭虫类似;采用已建立的针对血卵涡鞭虫ITS1基因的引物对"白浊病"病虾的血淋巴样品进行PCR检测,可扩增出585bp左右的特异条带。综合以上研究结果,确定该寄生虫为血卵涡鞭虫(Hematodinium sp.)。有关脊尾白虾感染该寄生虫的报道在国内外尚属首次。  相似文献   

银河系铝元素丰度研究     

马文娟  李宏杰  张波 《天文学报》2019,60(5):15-21

恒星的Al元素丰度可以为探索星团和星系的化学演化提供重要线索.通过系统分析银河系薄盘、厚盘、核球、银晕以及M4、M5等球状星团中恒星的[Al/Fe]随恒星金属丰度[Fe/H]的变化趋势,得出银河系薄盘、厚盘和核球恒星的[Al/Fe]随着[Fe/H]的增加而缓慢下降,而球状星团M4和M5恒星的[Al/Fe]随[Fe/H]增加没有下降趋势,这暗示Ia超新星对M4和M5恒星元素丰度的贡献比较小.详细研究了银河系恒星[Al/Fe]与[Mg/Fe]、[Na/Fe]的相关性,结果表明银河系场星的[Al/Fe]与[Mg/Fe]正相关,但在球状星团M4和M5恒星中未见此相关性;银河系盘星及M4和M5等球状星团恒星的[Al/Fe]与[Na/Fe]都存在正相关.  相似文献   

Spectroscopic study of the peculiar galaxy UGC 5119     

O. A. Merkulova  L. V. Shalyapina  V. A. Yakovleva  G. M. Karataeva 《Astronomy Letters》2008,34(8):542-550

We present the results of our study of the stellar kinematics in the elliptical galaxy UGC 5119, which has previously been suspected to be a polar-ring galaxy. We have detected a rapidly rotating disk in the central region (r ≤ 3.2 kpc) of the galaxy’s main body and found a radial velocity gradient along its minor axis (in the putative ring). We conclude that UGC 5119 is a medium-luminosity elliptical galaxy with a rapidly rotating disk component and a stellar (probably polar) ring. We have calculated the Lick indices of the Hβ, Mggb, Fe 5270, and Fe 5335 absorption lines and compared them with evolutionary synthesis models. Differences in the [Mg/Fe] ratios, metallicities, and ages of the stars have been found: the young stellar population with a solar [Mg/Fe] ratio and a high metallicity dominates in the circumnuclear region (r ≤ 1 kpc), while the old one with a low metal abundance dominates in the ring.  相似文献