Double radio peak and non-thermal collimated ejecta in RS Ophiuchi following the 2006 outburst     

S. P. S. Eyres  T. J. O'Brien  R. Beswick  T. W. B. Muxlow  G. C. Anupama  N. G. Kantharia  M. F. Bode  M. P. Gawro&#;ski  R. Feiler  A. Evans  M. T. Rushton  R. J. Davis  T. Prabhu  R. Porcas  B. J. M. Hassall 《Monthly notices of the Royal Astronomical Society》2009,395(3):1533-1540

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Baily’s Beads Atlas in 2005 – 2008 Eclipses     

C. Sigismondi  D. W. Dunham  K. Guhl  S. Andersson  H. Bode  O. Canales  P. Colona  O. Farago  M. Fernández-Ocaña  A. Gabel  M. Haupt  C. Herold  R. Nugent  P. Oliva  M. Patel  C. Perello  W. Rothe  J. Rovira  T. Schaefer  C. Schnabel  D. Schwartz  A. Selva  W. Strickling  A. Tegtmeier  C. Tegtmeier  B. Thome  W. H. Warren 《Solar physics》2009,258(2):191-202

In the annular or total eclipses of 3 October 2005, 29 March 2006, 22 September 2006, and 1 August 2008, observational campaigns were organized to record the phenomenon of Baily’s beads. These campaigns were internationally coordinated through the International Occultation Timing Association (IOTA) at both its American and European sections. From the stations in the northern and southern zones of grazing eclipse, the eclipses have been recorded on video. Afterward, as many beads as possible have been identified by analyzing the video data of each observing station. The atlas presented in this paper includes 598 data points, obtained by 23 observers operating at 28 different observing stations. The atlas lists the geographic positions of the observing stations and the observed time instants of disappearance or reappearance of beads, identified by an angle measured relative to the Moon’s axis of rotation. The atlas will serve as a basis for determining the solar diameter. Electronic Supplementary Material  The online version of this article () contains supplementary material, which is available to authorized users.  相似文献   

Changes in phytoplankton production and upwelling intensity off A Coruña (NW Spain) for the last 28 years     

Bode  Antonio  Álvarez  Marta  Ruíz-Villarreal  Manuel  Varela  Marta M. 《Ocean Dynamics》2019,69(7):861-873

Ocean Dynamics - The analysis of a 28-year-long (1989–2016) series of monthly measurements of chlorophyll concentrations and primary production rates at a shelf station off A Coruña (NW...  相似文献   

滇西保山地块金厂河矿集区铁铜金铅锌多金属矿床成矿系统          下载免费PDF全文

刘学龙  李文昌  周云满  赵成峰  王基元  李庆锐  李守奎  王海  陆波德  周杰虎  李方兰  刘雪 《沉积与特提斯地质》2022,42(1):133-150

滇西保山地块是西南"三江"特提斯构造带的重要组成部分,其大地构造位置处于藏-滇-泰-马中间板块中段,是近年来科学研究和地质找矿的热点地区之一.受区域构造演化的影响,保山地块先后历经原、古、中、新特提斯演化,并发生了多期成岩成矿事件,在北部形成了以金厂河铁铜铅锌矿、核桃坪铅锌矿、陡崖铁铜多金属矿、黑牛凹金矿、黄家地金矿等...  相似文献   

Direct observations of bipolar outflow from HM sagittae     

S. P. S. Eyres  R. J. Cohen  R. J. Davis  H. T. Kenny  H. M. Lloyd  M. F. Bode  S. M. Dougherty 《Astrophysics and Space Science》1995,224(1-2):457-458

We observed HM Sagittae with theMulti-Element Radio Linked Interferometer Network (MERLIN) at 6 cm and 18cm. We find non-thermal bipolar outflow in the eastwest direction, associated with optical emission lines, and thermal ridges to the north and south associated with the UV nebulosity detected by the HST.  相似文献   

High resolution radio images of the symbiotic system R aquarii     

S. M. Dougherty  M. F. Bode  H. M. Lloyd  R. J. Davis  S. P. Eyres 《Astrophysics and Space Science》1995,224(1-2):453-454

We present MERLIN images of the symbiotic system R Aquarii obtained at 1.7 and 5 GHz. We identify the emission from the binary system and derive a mass loss rate for the Mira that is commensurate with that in typical Miras. We show that variations in the radio emission over the last decade are consistent with the jet model for the system originally presented by Solf (1992). In addition, we calculate the spectral index distribution and find that there is no evidence of non-thermal emission.  相似文献   

Liverpool telescope 2: a new robotic facility for rapid transient follow-up     

C. M. Copperwheat  I. A. Steele  R. M. Barnsley  S. D. Bates  D. Bersier  M. F. Bode  D. Carter  N. R. Clay  C. A. Collins  M. J. Darnley  C. J. Davis  C. M. Gutierrez  D. J. Harman  P. A. James  J. H. Knapen  S. Kobayashi  J. M. Marchant  P. A. Mazzali  C. J. Mottram  C. G. Mundell  A. Newsam  A. Oscoz  E. Palle  A. Piascik  R. Rebolo  R. J. Smith 《Experimental Astronomy》2015,39(1):119-165

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The effect of the "Prestige" oil spill on the plankton of the N-NW Spanish coast     

Varela M  Bode A  Lorenzo J  Alvarez-Ossorio MT  Miranda A  Patrocinio T  Anadón R  Viesca L  Rodríguez N  Valdés L  Cabal J  Urrutia A  García-Soto C  Rodríguez M  Alvarez-Salgado XA  Groom S 《Marine pollution bulletin》2006,53(5-7):272-286

Chlorophyll, primary production, zooplankton biomass and the species composition of phytoplankton and zooplankton were studied in 2003, after the Prestige shipwreck. The information obtained was compared to previous data series available for the area affected by the spill. A large data series on plankton variables for the N-NW Spanish coast existed, and therefore a realistic evaluation of the effects by comparison with the range of natural variability could be carried out. We emphasized the evaluation of impact during the spring bloom, the first important biological event after the spill. Some minor changes were observed occasionally, but they did not show any clear pattern and were more related to the natural variability of the ecosystem than to effect of the spill. Plankton community structure did not undergo any changes. Only a few species were more abundant during spring 2003 than in previous years. No significant changes were detected in the planktonic community during productive periods, such as the spring bloom and the summer blooms related to intrusions of East North Atlantic Central Waters. The lack of evidence of the effects of the spill on planktonic communities is discussed in terms of the characteristics of the fuel, the high dynamics of the water masses, the biological mechanisms through which the fuel from the surface waters is transferred to the sea floor and, particularly, the influence of the natural variability by means of large and meso-scale hydrographic processes in the area under study. At the present time it is not possible to determine any minor effects the spill may have had on the plankton owing to the great variability of the planktonic cycles and the short-term impact of the oil from the Prestige on the pelagic system.  相似文献   

The outbursts of classical and recurrent novae     

M.F. Bode 《Astronomische Nachrichten》2010,331(2):160-168

In this review, I present our current state of knowledge regarding both Classical Nova and Recurrent Nova systems. Two particular objects (V1974 Cyg and RS Oph) are chosen to illustrate the range of phenomena that may be associated with their outbursts. The wider importance of nova research is emphasised and some of the most pressing unsolved problems are summarised (© 2010 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

On the asphericity of nova remnants caused by rotating white dwarf envelopes     

John M. Porter  O'Brien  & Mike F. Bode 《Monthly notices of the Royal Astronomical Society》1998,296(4):943-948

The effect of rotating white dwarf envelopes in determining the structure of nova shells is examined. This is achieved by numerical hydrodynamic simulations of the flows around a binary star system. In previous studies of remnant formation, this rotation has not been included.
It is found that the structures formed in the flow are more consistent with observations of nova shells than the previous theoretical studies. The shells produced by the nova become more prolate with increasing white dwarf envelope rotation. Hence the rotation of white dwarf envelopes must be included in any future discussion of remnant formation.
A possible method of identifying the dominant process by which mixing of accreted and white dwarf matter takes place is suggested.  相似文献