Giant Lyα nebulae around z > 2 radio galaxies: evidence for infall     

A. Humphrey  M. Villar-Martín  R. Fosbury  L. Binette  J. Vernet  C. De Breuck  S. di Serego Alighieri 《Monthly notices of the Royal Astronomical Society》2007,375(2):705-714

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The young star cluster system in the Antennae: evidence for a turnover in the luminosity function     

P. Anders  N. Bissantz  L. Boysen  R. de Grijs  U. Fritze-v.Alvensleben 《Monthly notices of the Royal Astronomical Society》2007,377(1):91-106

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长三角房价收入比时空演变格局及收敛性研究   总被引：2，自引：1，他引：2  

尹上岗  杨山  陈艳如  白彩全 《地理研究》2020,39(11):2521-2536

房价收入比是衡量房地产健康状况和探测居民住房支付能力的重要指标。以2008—2018年长三角307个区县为研究单元,运用数值-位序法则和趋势面分析对房价收入比的总体分布特征进行探究,利用LISA时间路径分析房价收入比的时空动态性特征,并检验区域房价收入比的收敛性。结果表明： ① 长三角房价收入比总体上呈上升趋势,空间上表现为东高西低、南高北低的格局,上海、浙江、江苏和安徽依次降低。② 上海和浙江南部房价收入比的空间结构更具动态性,而江苏和安徽更加稳定;长三角房价收入比的空间演化整体上具有较强的空间锁定效应和空间整合性。③ 长三角区县房价收入比整体上不存在σ收敛,但各时间段上均存在显著的绝对β收敛,且各省份内部也均存在着俱乐部收敛现象。城市群房价收入比的变动对居民的流动有着重要的指示作用,并具有扩散效应和虹吸效应。加强城市群房地产市场一体化建设,是促进城市群区域一体化发展的有效途径。  相似文献   

The born-again (very late thermal pulse) scenario revisited: the mass of the remnants and implications for V4334 Sgr     

M. M. Miller Bertolami  L. G. Althaus 《Monthly notices of the Royal Astronomical Society》2007,380(2):763-770

We present 1D numerical simulations of the very late thermal pulse (VLTP) scenario for a wide range of remnant masses. We show that by taking into account the different possible remnant masses, the observed evolution of V4334 Sgr (a.k.a. Sakurai's object) can be reproduced within the standard 1D mixing length theory (MLT) stellar evolutionary models without the inclusion of any ad hoc reduced mixing efficiency. Our simulations hint at a consistent picture with present observations of V4334 Sgr. From energetics, and within the standard MLT approach, we show that low-mass remnants  ( M ≲ 0.6 M_⊙)  are expected to behave markedly differently from higher mass remnants  ( M ≳ 0.6 M_⊙)  in the sense that the latter remnants are not expected to expand significantly as a result of the violent H-burning that takes place during the VLTP. We also assess the discrepancy in the born-again times obtained by different authors by comparing the energy that can be liberated by H-burning during the VLTP event.  相似文献   

Star formation and figure rotation in the early-type galaxy NGC 2974     

Hyunjin Jeong  Martin Bureau  Sukyoung K. Yi  Davor Krajnovi&#;  Roger L. Davies 《Monthly notices of the Royal Astronomical Society》2007,376(3):1021-1032

We present Galaxy Evolution Explorer ( GALEX ) far-ultraviolet (FUV) and near-ultraviolet (NUV) imaging of the nearby early-type galaxy NGC 2974, along with complementary ground-based optical imaging. In the ultraviolet, the galaxy reveals a central spheroid-like component and a newly discovered complete outer ring of radius 6.2 kpc, with suggestions of another partial ring at an even larger radius. Blue FUV–NUV and UV-optical colours are observed in the centre of the galaxy and from the outer ring outwards, suggesting young stellar populations (≲1 Gyr) and recent star formation in both locations. This is supported by a simple stellar population model which assumes two bursts of star formation, allowing us to constrain the age, mass fraction and surface mass density of the young component pixel by pixel. Overall, the mass fraction of the young component appears to be just under 1 per cent (lower limit, uncorrected for dust extinction). The additional presence of a nuclear and an inner ring (radii 1.4 and 2.9 kpc, respectively), as traced by [O  iii ] emission, suggests ring formation through resonances. All three rings are consistent with a single pattern speed of  78 ± 6  km s⁻¹ kpc⁻¹, typical of S0 galaxies and only marginally slower than expected for a fast bar if traced by a small observed surface brightness plateau. This thus suggests that star formation and morphological evolution in NGC 2974 at the present epoch are primarily driven by a rotating asymmetry (probably a large-scale bar), despite the standard classification of NGC 2974 as an E4 elliptical.  相似文献   

2003-2017年北京市地表热力景观时空分异特征及演变规律   总被引：6，自引：3，他引：6  

乔治  黄宁钰  徐新良  孙宗耀  吴晨  杨俊 《地理学报》2019,74(3):475-489

利用2003-2017年MODIS地表温度数据,分别从数量、形状和结构角度揭示北京市不同季相和昼夜间地表热力景观时空分异特征,并进一步通过热力等级变化图谱及质心迁移轨迹揭示城市热力景观空间演变规律,探究热力景观等级转换生态过程。结论如下：① 城市地表热力景观季节和昼夜空间特征差异显著;② 中温区在城市热环境中占主导地位。白天中温区是最不稳定的热力景观等级;夜间次低温区和次高温区不稳定性增加;③ 地表热力景观等级变化以稳定型占主,反复变化型和前期变化型次之。地表热力景观等级通常呈现逐级递增或递减规律,山区呈现逐级降温趋势,北部城郊—山地交错地带表现出次低温和中温的反复转向,南部地区有一定的升温趋势;④ 2003-2017年高温区面积增大且质心向城市中心集中,低温区质心向城市外围扩散。生态涵养发展区对北京市地表热力景观质心迁移贡献率最高。热力景观时空分异特征及演变规律可为有效缓解城市热岛效应提供管理决策支持。  相似文献   

Abundance diagnosis of E+A (post-starburst) galaxies   总被引：1，自引：0，他引：1  

Tomotsugu Goto 《Monthly notices of the Royal Astronomical Society》2007,377(3):1222-1228

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Gemini GMOS/integral field unit spectroscopy of NGC 1569 – II. Mapping the roots of the galactic outflow     

M. S. Westmoquette  L. J. Smith  J. S. Gallagher III    K. M. Exter † 《Monthly notices of the Royal Astronomical Society》2007,381(3):913-931

We present a set of four Gemini-North Multi-Object Spectrograph/integral field unit (IFU) observations of the central disturbed regions of the dwarf irregular starburst galaxy NGC 1569, surrounding the well-known superstar clusters A and B. This continues on directly from a companion paper, in which we describe the data reduction and analysis techniques employed and present the analysis of one of the IFU pointings. By decomposing the emission-line profiles across the IFU fields, we map out the properties of each individual component identified and identify a number of relationships and correlations that allow us to investigate in detail the state of the ionized interstellar medium (ISM). Our observations support and expand on the main findings from the analysis of the first IFU position, where we conclude that a broad (≲400 km s⁻¹) component underlying the bright nebular emission lines is produced in a turbulent mixing layer on the surface of cool gas knots, set up by the impact of the fast-flowing cluster winds. We discuss the kinematic, electron-density and excitation maps of each region in detail and compare our results to previous studies. Our analysis reveals a very complex environment with many overlapping and superimposed components, including dissolving gas knots, rapidly expanding shocked shells and embedded ionizing sources, but no evidence for organized bulk motions. We conclude that the four IFU positions presented here lie well within the starburst region where energy is injected, and, from the lack of substantial ordered gas flows, within the quasi-hydrostatic zone of the wind interior to the sonic point. The net outflow occurs at radii beyond 100–200 pc, but our data imply that mass-loading of the hot ISM is active even at the roots of the wind.  相似文献   

The SAURON project – IX. A kinematic classification for early-type galaxies     

Eric Emsellem  Michele Cappellari  Davor Krajnovi&#;  Glenn van de Ven  R. Bacon  M. Bureau  Roger L. Davies  P. T. de Zeeuw  Jesús Falcón-Barroso  Harald Kuntschner  Richard McDermid  Reynier F. Peletier  Marc Sarzi 《Monthly notices of the Royal Astronomical Society》2007,379(2):401-417

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An alternative to common envelope evolution     

Martin E. Beer  Lynnette M. Dray  rew R. King  Graham A. Wynn 《Monthly notices of the Royal Astronomical Society》2007,375(3):1000-1008

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