A comprehensive CCD photometric study of the open cluster NGC 2421     

R. K. S. Yadav  Ram Sagar 《Monthly notices of the Royal Astronomical Society》2004,351(2):667-675

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Imaging study of NGC 3372, the Carina nebula – II. Evidence of activity in the complex Trumpler 14/Car I photodissociation region     

M. Tapia  P. Persi  J. Bohigas  M. Roth  M. Gómez 《Monthly notices of the Royal Astronomical Society》2006,367(2):513-526

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Composite spectra Paper 14: HR 1129, a long-period binary showing evidence of circumbinary material     

R. E. M. Griffin †  R. F. Griffin †  D. J. Stickland † 《Monthly notices of the Royal Astronomical Society》2006,373(4):1351-1368

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掌鳞刺属演化及晚泥盆世环境变迁     

王超勇  夏文臣 《南方国土资源》2002,15(2):21-25

牙形石掌鳞刺属Palmatolepis齿台结构和形态随时间演替 ,由近正三角形向长三角形、长菱形演化 ,在F/F界线附近受地质事件的影响而中断 ,使Palmatolepis齿台结构呈二段式发展 ,在Palmatolepis的分子中 ,那些演化速度快 ,结构变化大的分子首先灭绝 ,而那些演化速度慢 ,结构变化小的分子延续时间长 ,分布范围也更加广泛 ,在地质事件中被保留下来并得以延续 ,这种演化规律可能是生物有选择性灭绝与复苏的原因之一。晚泥盆世F/F之交环境的变化可能是由于海退 ,海底毒气喷发 ,超量金属元素的污染造成的  相似文献   

Molecular line mapping of the giant molecular cloud associated with RCW 106 – I. ¹³CO     

I. Bains  T. Wong  M. Cunningham  P. Sparks  D. Brisbin  P. Calisse  J. T. Dempsey  G. Deragopian  S. Ellingsen  B. Fulton  F. Herpin  P. Jones  Y. Kouba  C. Kramer  E. F. Ladd  S. N. Longmore  J. McEvoy  M. Maller  V. Minier  B. Mookerjea  C. Phillips  C. R. Purcell  A. Walsh  M. A. Voronkov  M. G. Burton 《Monthly notices of the Royal Astronomical Society》2006,367(4):1609-1628

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Molecular Gas and Dust in the Massive Star Forming Region S 233 IR     

Rui-Qing Mao  Qin Zeng Purple Mountain Observatory  Chinese Academy of Sciences  Nanjing  National Astronomical Observatories  Chinese Academy of Sciences  Beijing 《中国天文和天体物理学报》2004,4(5):440-454

The massive star forming region S 233 IR is observed in the molecular lines CO J = 2-1, 3-2, NH3 (1,1), (2,2) and the 870#m dust continuum. Four submillimeter continuum sources, labelled SMM 1-4, are revealed in the 870μm dust emission. The main core, SMM1, is found to be associated with a deeply embedded near infrared cluster in the northeast; while the weaker source SMM2 coincides with a more evolved cluster in the southwest. The best fit spectral energy distribution of SMM1 gives an emissivity of β = 1.6, and temperatures of 32 K and 92 K for the cold- and hot-dust components. An SMM1 core mass of 246 M⊙ and a total mass of 445 M⊙ are estimated from the 870μm dust continuum emission.SMM1 is found to have a temperature gradient decreasing from inside out, indicative of the presence of interior heating sources. The total outflow gas mass as traced by the CO J = 3-2 emission is estimated to be 35 M⊙. Low velocity outflows are also found in the NH3 (1,1) emission. The non-thermal dominant NH3 line width as well as the substantial core mass suggest that the SMM1 core is a “turbulent,massive dense core”, in the process of forming a group or a cluster of stars. The much higher star formation efficiency found in the southwest cluster supports the suggestion that this cluster is more evolved than the northeast one. Large near infrared photometric variations found in the source PCS-IR93, a previously found highly polarized nebulosity, indicate an underlying star showing the FU Orionis type of behavior.  相似文献   

Properties of dust and detection of Hα emission in LDN 1780     

C. del Burgo  L. Cambrésy 《Monthly notices of the Royal Astronomical Society》2006,368(3):1463-1478

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On the mixing rules for astrophysical inhomogeneous grains     

N. Maron  O. Maron 《Monthly notices of the Royal Astronomical Society》2005,357(3):873-880

We present the computation of effective refractive coefficients for inhomogeneous two-component grains with three kinds of inclusions with   m _incl= 3.0 + 4.0i, 2.0 + 1.0i, 2.5 + 0.0001i  and a matrix with   m_m = 1.33 + 0.01i  for 11 volume fractions of inclusions from 0 to 50 per cent and wavelengths  λ= 0.5  , 1.0, 2.0 and 5.0 μm. The coefficients of extinction for these grains have been computed using a discrete dipole approximation. Computation of the extinction by the same method for grains composed of a matrix material with randomly embedded inclusions has been carried out for different volume fractions of inclusions. A comparison of extinction coefficients obtained for both models of grain material allows one to choose the best mixing rule for a mixture. In cases of inclusions with   m _incl= 2.0 + 1.0i  and 2.5 + 0.0001i the best fit for the whole wavelength range and volume fractions of inclusions from 0 to 50 per cent has been obtained for the Lichtenecker mixing rule. In the case of   m _incl= 3.0 + 4.0i  the fit for the whole wavelength range and volume fractions of inclusions from 0 to 50 per cent is not very significant but the best fit has been obtained for the Hanai rule. For volume fractions of inclusions from 0 to 15 per cent a very good fit has been obtained for the whole wavelength range for Rayleigh and Maxwell-Garnett mixing rules.  相似文献   

Extremely red galaxies: dust attenuation and classification     

D. Pierini  C. Maraston  R. Bender  A. N. Witt 《Monthly notices of the Royal Astronomical Society》2004,347(1):1-16

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Submillimetre observations of z > 6 quasars     

Ian Robson  Robert S. Priddey  Kate G. Isaak  Richard G. McMahon 《Monthly notices of the Royal Astronomical Society》2004,351(2):L29-L33

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