数字滤波技术在射电天文测量中的应用     

项英  张秀忠 《天文学进展》2004,22(2):95-103

随着数字技术的发展，数字信号处理芯片的速度越来越快，这为高速数字滤波的实时实现提供了可能。简要阐述了数字滤波的原理，并对两种数字滤波的实现方法进行了分析；给出了数字滤波较模拟滤波的优势；介绍了数字滤波在射电天文测量中的各种应用。  相似文献   

The electron temperature and density in interstellar medium by using carbon radio recombination line observations     

N.I. Rovenskaya 《Astrophysics and Space Science》2004,291(2):113-122

The intensities of carbon radio recombination lines (RRL’s) are definedallowing for the effect of dielectronic-like recombination. The rate ofdielectronic-like recombination is calculated as functions of line number,electron density and temperature accurate to 0.05. Following from the balanceequation solutions for populations, the RRL intensities are analytically foundby the method of successive approximations to an accuracy of 0.15. Theobservations of carbon RRL’s are analyzed toward Cassiopeia A. The averageelectron temperature, density, expanded CII region lengths and inaccuraciesare found with the experimental values of RRL widths and intensities.  相似文献   

Relativistic models of two low-luminosity radio jets: B2 0326+39and B2 1553+24   总被引：1，自引：0，他引：1  

J.R. Canvin  R. A. Laing 《Monthly notices of the Royal Astronomical Society》2004,350(4):1342-1365

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Helical magnetic fields associated with the relativistic jets of four BL Lac objects     

Denise C. Gabuzda  Éamonn Murray  Patrick Cronin 《Monthly notices of the Royal Astronomical Society》2004,351(4):L89-L93

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Visibility of old supernova remnants in H i 21-cm emission line     

Bon-Chul Koo  Ji-hyun Kang 《Monthly notices of the Royal Astronomical Society》2004,349(3):983-993

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射电天球参考架指向维持方法讨论     

李金岭  金文敬  李金增 《天文研究与技术》1994,(4)

依据河外射电源天球参考架的现状与建立射电天球参考架的最终目的，本文提出了以共同基本源维持参考架指向的观点。对实际资料的归算结果表明，在确保参考架指向长期稳定性方面，共同基本源指向维持模型优于ＩＥＲＳ维持模型。依据验算结果，文中同时讨论了选源标准与参考架指向稳定性的关系，指出基本源一次性变更的比例不能过高。一方面应完善选源标准；另一方面，一旦此标准发生性？上的改变时，应对在旧标准下选出的基本源进行复核，并作相应的指向调整，否则将可能造成参考架指向的跳变。  相似文献   

Global very long-baseline interferometry observations of compact radio sources in M82     

A. R. McDonald  T. W. B. Muxlow  A. Pedlar  M. A. Garrett  K. A. Wills  S. T. Garrington  P. J. Diamond  P. N. Wilkinson 《Monthly notices of the Royal Astronomical Society》2001,322(1):100-106

Observations of the starburst galaxy, M82, have been made with a 20-station global very long-baseline interferometry (VLBI) array at λ 18 cm. Maps are presented of the brightest young supernova remnants (SNR) in M82 and the wide-field mapping techniques used in making images over a field of view of ∼1 arcmin with 3-milliarcsecond resolution are discussed. A limit has been placed on the power-law deceleration of the young supernova remnant (SNR) 43.31+592 with an index greater than 0.73±0.11 from observations with the European VLBI Network. Using the global array we have resolved compact knots of radio emission in the source which, with future global observations, will enable better constraints to be placed on the expansion parameters of this SNR.
The latest global observations have also provided high-resolution images of the most compact radio source in M82, 41.95+575. We determine an upper limit to the radial expansion rate along the major axis of 2000 km s⁻¹. However, the new images also show structure resembling that of collimated ejection which brings into question the previous explanation of the source as being a result of the confinement of a supernova by a high-density circumstellar medium.
It is apparent that we are now able to image the brightest supernova remnants in M82 with a linear scale which allows direct comparison with galactic SNR such as Cassiopeia A.  相似文献   

EVN observations of low-luminosity flat-spectrum active galactic nuclei     

A. Caccianiga  M.J.M. Marchã  A. Thean  J. Dennett-Thorpe 《Monthly notices of the Royal Astronomical Society》2001,328(3):867-872

We present and discuss the results of very-long baseline interferometry (VLBI, EVN) observations of three low-luminosity     broad emission line active galactic nuclei (AGNs) carefully selected from a sample of flat-spectrum radio sources (CLASS). Based on the total and the extended radio power at 5 and at 1.4 GHz respectively, these objects should be technically classified as radio-quiet AGN and thus the origin of their radio emission is not clearly understood. The VLBI observations presented in this paper have revealed compact radio cores which imply a lower limit on the brightness temperature of about     . This result rules out a thermal origin for the radio emission and strongly suggests an emission mechanism similar to that observed in more powerful radio-loud AGNs. Since, by definition, the three objects show a flat (or inverted) radio spectrum between 1.4 and 8.4 GHz, the observed radio emission could be relativistically beamed. Multi-epoch VLBI observations can confirm this possibility in two years' time.  相似文献   

The LBDS Hercules sample of mJy radio sources at 1.4 GHz – II. Redshift distribution, radio luminosity function, and the high-redshift cut-off     

I. Waddington †  J.S. Dunlop  J.A. Peacock  R.A. Windhorst 《Monthly notices of the Royal Astronomical Society》2001,328(3):882-896

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A Parkes half-Jansky sample of GHz peaked spectrum galaxies     

I. A. G. Snellen  M. D. Lehnert  M. N. Bremer  R. T. Schilizzi 《Monthly notices of the Royal Astronomical Society》2002,337(3):981-992

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