从地理空间到地理网络空间的变化趋势--兼论西方学者关于电信对地区影响的研究

信息通信技术(ICTs)正切实地影响着人类和社会状况:网络空间的出现和电信压缩空间使距离屏障失去意义.通过对西方学者过去十余年的主要探索成就进行综合.将评价电信在地区发展中作用的研究观点划分为三类,并分别予以评述.我们认为当前地理空间和网络空间交织在一起,处于一种融合过程,可把它叫做"地理网络空间".电信在地区发展和行为区位方面的作用及特殊优势仍有待于进一步研究.     

从地理空间到地理网络空间的变化趋势：兼论西方学者关于电信对地？…

信息通信技术（ＩＣＴｓ）正切实地影响着人类和社会状况：网络空间的出现和曜压缩空间使距离屏障失去意义。通过对西方学者过去十余年的主要探索成就进行综合。将评价电信在中地区发展中作用的研究观点划分为三类,并分别予以评述。我们认为当前地理空间和网络空间交织在一起,处于一种融合过程,可把它叫做“地理网络空间”。电信在地区发展和行闰方面的作用及特殊优势仍有待于进一步研究。     

Astrometric Solution of the Multiple System Xy Leo

An astrometric solution, together with time of minimum analysis, has been made for the multiple system XY Leonis (HIP 49136) to identify the properties of the remote companion to the eclipsing pair (AB). From this solution, we derive the inclination of the wide orbit (AB-cd) as 94.4^∘± 0.2^∘, angle of nodes as 247.3^∘± 0.2^∘, and the mass of the wide component (the dwarf binary cd) as 0.98 ± 0.2 M_⊙. This study confirms that the light travel time effect can explain the sinusoidal O−C variation of the eclipsing system.     

Multi-Facility Study of the Algol-Type Binary δ Librae

Various branches of observational information, and related physical problems concerning the bright, relatively close, Algol binary δ Lib are discussed. Times of minimum light confirm the classical Algol status, which, combined with the optical and IR photometry of Lazaro et al. (2002), provide the basis for a good understanding of the system’s basic parameters. New spectroscopy from the Coudé spectrograph of the Rozhen Observatory (Bulgaria) allows further information on the model and the mass transfer process. Very high resolution radio observations would also have much to reveal about astrophysics of the semi-detached configuration, not only directly, by informing about the outermost envelopes of the components, but indirectly through high accuracy positional information. We show how this may be related to careful period and astrometric studies. δ Lib thus provides a rich source of information on the astrophysics of the Algol configuration.     

First ground‐based photometry and light‐curve analysis of the eccentric eclipsing binary V744 Cas

The first ground‐based BVR photometric observations of the recently discovered eclipsing binary V744 Cas are presented. From these measurements, timings for two primary and one secondary minima have been calculated. The light curves of the system were analyzed by using the Wilson‐Devinney program. The analysis shows that the system is detached with two similar components of spectral type A2V, and the orbit is eccentric (e = 0.0662 ± 0.0005). The longitude of the periastron (ω) was found significantly different for two different light curves (ours and that of Hipparcos), which is strongly suggestive of an apsidal motion with a period of about 425 ± 68 yr. This makes V744 Cas an important candidate for studies of apsidal motions. The first estimate of the absolute dimensions place the system close to the terminal age of the main sequence (TAMS) in the HR diagram. The distance from the spectroscopic parallax (d = 740 ± 10 pc) was found to be slightly larger than the Hipparcos distance of d = 610 ± 400 pc. (© 2006 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)