Low‐mass visual binaries in the solar neighbourhood: The case of HD 141272     

T. Eisenbeiss  A. Seifahrt  M. Mugrauer  T. O. B. Schmidt  R. Neuhuser  T. Roell 《Astronomische Nachrichten》2007,328(6):521-526

We search for stellar and substellar companions of young nearby stars to investigate stellar multiplicity and formation of stellar and substellar companions. We detect common proper‐motion companions of stars via multi‐epoch imaging. Their companionship is finally confirmed with photometry and spectroscopy. Here we report the discovery of a new co‐moving (13 σ) stellar companion ∼17.8 arcsec (350AU in projected separation) north of the nearby star HD141272 (21 pc).With EMMI/NTT optical spectroscopy we determined the spectral type of the companion to be M3±0.5V. The derived spectral type as well as the near infrared photometry of the companion are both fully consistent with a M_⊙ dwarf located at the distance of HD141272 (21 pc). Furthermore the photometry data rules out the pre‐main sequence status, since the system is consistent with the ZAMS of the Pleiades. (© 2007 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

A near‐infrared/optical/X‐ray survey in the centre of σ Orionis     

J.A. Caballero 《Astronomische Nachrichten》2007,328(9):917-927

Because of the intense brightness of the OB‐type multiple star system σ Ori, the low‐mass stellar and substellar populations close to the centre of the very young σ Orionis cluster is poorly know. I present an IJHK_s survey in the cluster centre, able to detect from the massive early‐type stars down to cluster members below the deuterium burning mass limit. The near‐infrared and optical data have been complemented with X‐ray imaging. Ten objects have been found for the first time to display high‐energy emission. Previously known stars with clear spectroscopic youth indicators and/or X‐ray emission define a clear sequence in the I vs. I – K_s diagram. I have found six new candidate cluster members that follow this sequence. One of them, in the magnitude interval of the brown dwarfs in the cluster, displays X‐ray emission and a very red J – K_s colour, indicative of a disc. Other three low‐mass stars have excesses in the K_s band as well. The frequency of X‐ray emitters in the area is 80±20 %. The spatial density of stars is very high, of up to 1.6±0.1 arcmin^–2. There is no indication of lower abundance of substellar objects in the cluster centre. Finally, I also report two cluster stars with X‐ray emission located at only 8000–11000 AU to σ Ori AB, two sources with peculiar colours and an object with X‐ray emission and near‐infrared magnitudes similar to those of previously‐known substellar objects in the cluster. (© 2007 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

High proper motion stars in Kapteyn Selected Area 94     

J. A. Cooke  I. Neill Reid 《Monthly notices of the Royal Astronomical Society》2000,318(4):1206-1216

We have applied the astrometric techniques devised by Murray for analysis of 48-inch Schmidt photographic data to SuperCOSMOS scans of UK Schmidt plates centred on Kapteyn's Selected Area 94 ( α =2^h 53^m, δ =0°). In this preliminary study, we combine astrometric data from four short-exposure V -band plates, taken in 1987 August (2 plates) and 1993 August (2 plates), with BVRI photometry from sky-limited plate material, to identify stars with proper motions exceeding 0.1 arcsec yr⁻¹. This paper discusses the completeness of the resulting sample and presents spectroscopy of 30 stars with μ >0.2 arcsec yr⁻¹. Based on the latter observations and the distribution in the [H _V , ( V − I )] reduced proper-motion diagram, we have classified stars in the complete sample as candidate white dwarfs, main-sequence dwarfs and halo subdwarfs, and derived estimates of the disc and halo luminosity functions.  相似文献   

On the late spectral types of cataclysmic variable secondaries     

I. Baraffe  U. Kolb 《Monthly notices of the Royal Astronomical Society》2000,318(2):354-360

We investigate why the spectral type of most cataclysmic variable (CV) secondaries is significantly later than that of a zero-age main-sequence (ZAMS) star with the same mean density. Using improved stellar input physics, tested against observations of low-mass stars at the bottom of the main sequence, we calculate the secular evolution of CVs with low-mass donors. We consider sequences with different mass transfer rates and with a different degree of nuclear evolution of the donor prior to mass transfer.
Systems near the upper edge of the gap ( P ∼3–6 h) can be reproduced by models with a wide range of mass transfer rates from 1.5×10⁻⁹ M_⊙ yr⁻¹ to 10⁻⁸ M_⊙ yr⁻¹. Evolutionary sequences with a small transfer rate and donors that are substantially evolved off the ZAMS (central hydrogen content 0.05–0.5) reproduce CVs with late spectral types above P ≳6 h. Systems with the most discrepant (late) spectral type should have the smallest donor mass at any given P .
Consistency with the period gap suggests that the mass transfer rate increases with decreasing donor mass for evolved sequences above the period gap. In this case, a single-parameter family of sequences with varying X _c and increasing mass transfer rate reproduces the full range of observed spectral types. This would imply that CVs with such evolved secondaries dominate the CV population.  相似文献   

长江中下游黄棕壤中若干元素的环境地球化学特征   总被引：3，自引：1，他引：2  

洪松  陈静生  周智强  王少平  龙泉  郑泽厚 《地理科学》2000,20(4):320-325

在长江中下游黄棕壤上采集１２９个土样,测定了其中１４种元素（１３种微量元素和Ｆｅ）的全量含量,比较了不同岩石上发育的黄棕壤元素含量的差异,分析了其剖面分布特征。讨论了目前农业生产中广泛关注的５种微量元素和Ｆｅ的有效态含量在黄棕壤剖面中的迁移分布及其影响因素。  相似文献   

从藻类化石的垂直分布探讨杭州西湖的演变历程   总被引：4，自引：0，他引：4  

项斯端  赵建康  周宏  王江毅 《海洋与湖沼》1999,30(1):14-24

于１９９４年春在杭州西湖东北面,西面及湖中心小瀛洲３个钻孔共取了７０号岩芯样,经浮选,筛选,以显微镜检鉴定化石藻种,并分析其垂直分布,从而探讨西湖的形成历史,西湖自晚更新世以来的６个化石藻带由下而上依次为：轮藻带,微藻带,微红金颗藻－近缘针杆藻－条纹小环藻带,圆筛藻带,圆筛藻－近缘针杆藻－微红金颗藻桥穹藻－异极藻－短缝藻带和水花束丝藻带,从而反映了西湖的６个发育时期,淡水古湖沼期,淡咸水过渡期,海  相似文献   

Brown dwarfs in the Pleiades and the initial mass function across the stellar/substellar boundary     

N. C. Hambly  S. T. Hodgkin  M. R. Cossburn  R. F. Jameson 《Monthly notices of the Royal Astronomical Society》1999,303(4):835-844

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The effect of sewage plant effluent on brown trout (Salmo trutta fario): a cage experiment     

Matthias Escher  Thomas Wahli  Sabina Büttner  Willy Meier  Patricia Burkhardt-Holm 《Aquatic Sciences - Research Across Boundaries》1999,61(2):93-110

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Astrometric confirmation of a wide low‐mass companion to the planet host star HD 89744     

M. Mugrauer  R. Neuhuser  T. Mazeh  E. Guenther  M. Fernndez 《Astronomische Nachrichten》2004,325(9):718-722

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西沙群岛原绿藻的超微构造研究     

孙爱淑  曾呈奎 《海洋与湖沼》1998,29(4):347-352

于1981年3月在西沙群岛永兴岛采集原绿藻标本。用光镜和电镜对所采原绿藻进行研究。结果表明,原绿藻为简单的原核、单细胞藻类,在同一生境的相同宿主体表有4种不同的细胞构造类型：第1种类型,中央大“液泡”,类囊体单条、平行分散于周围区的细胞质中;第2种类型,中央是大“液泡”,周围区内类囊体多,并形成垛叠;第3种类型,许多小泡充满细胞的大部分,类囊体穿插于小泡之间;第4种类型,有中央大“液泡”,还有许多小泡分散在细胞周围区。上述分类以类囊体和“液泡”的结构和分布为主要分类依据,反映出不同结构的进化意义。表明中国西沙群岛有丰富的原绿藻资源。  相似文献