全文获取类型
收费全文 | 582篇 |
免费 | 25篇 |
国内免费 | 7篇 |
专业分类
测绘学 | 21篇 |
大气科学 | 37篇 |
地球物理 | 130篇 |
地质学 | 196篇 |
海洋学 | 65篇 |
天文学 | 102篇 |
综合类 | 3篇 |
自然地理 | 60篇 |
出版年
2021年 | 7篇 |
2020年 | 11篇 |
2019年 | 16篇 |
2018年 | 15篇 |
2017年 | 15篇 |
2016年 | 19篇 |
2015年 | 12篇 |
2014年 | 16篇 |
2013年 | 34篇 |
2012年 | 12篇 |
2011年 | 35篇 |
2010年 | 11篇 |
2009年 | 23篇 |
2008年 | 24篇 |
2007年 | 30篇 |
2006年 | 24篇 |
2005年 | 24篇 |
2004年 | 20篇 |
2003年 | 9篇 |
2002年 | 16篇 |
2001年 | 22篇 |
2000年 | 15篇 |
1999年 | 14篇 |
1998年 | 7篇 |
1997年 | 7篇 |
1996年 | 4篇 |
1995年 | 5篇 |
1994年 | 5篇 |
1993年 | 10篇 |
1992年 | 12篇 |
1991年 | 9篇 |
1990年 | 4篇 |
1989年 | 9篇 |
1988年 | 6篇 |
1987年 | 10篇 |
1986年 | 4篇 |
1985年 | 7篇 |
1984年 | 10篇 |
1983年 | 6篇 |
1982年 | 6篇 |
1981年 | 4篇 |
1980年 | 7篇 |
1978年 | 7篇 |
1976年 | 4篇 |
1975年 | 8篇 |
1973年 | 5篇 |
1972年 | 3篇 |
1971年 | 5篇 |
1970年 | 5篇 |
1969年 | 3篇 |
排序方式: 共有614条查询结果,搜索用时 15 毫秒
81.
A.J. Young † A.C. Fabian R.R. Ross Y. Tanaka 《Monthly notices of the Royal Astronomical Society》2001,325(3):1045-1052
The galactic black hole candidate Cygnus X-1 is observed to be in one of two X-ray spectral states: either the low/hard (low soft X-ray flux and a flat power-law tail) or high/soft (high blackbody-like soft X-ray flux and a steep power-law tail) state. The physical origin of these two states is unclear. We present here a model of an ionized accretion disc, the spectrum of which is blurred by relativistic effects, and fit it to the ASCA , Ginga and EXOSAT data of Cygnus X-1 in both spectral states. We confirm that relativistic blurring provides a much better fit to the low/hard state data and, contrary to some previous results, find the data of both states to be consistent with an ionized thin accretion disc with a reflected fraction of unity extending to the innermost stable circular orbit around the black hole. Our model is an alternative to those that, in the low/hard state, require the accretion disc to be truncated at a few tens of Schwarzschild radii, within which there is a Thomson-thin, hot accretion flow. We suggest a mechanism that may cause the changes in spectral state. 相似文献
82.
83.
Alexander Deutsch Christian Koeberl Joel D. Blum Bevan M. French Billy P. Glass Richard Grieve Peter Horn Elmar K. Jessberger Gero Kurat Wolf Uwe Reimold Jan Smit Dieter Stöffler Stuart Ross Taylor 《地学学报》1994,6(6):644-650
In a recent article in Terra Nova, Kristan-Tollmann and Tollmann (1994) suggested that the Biblical Flood can be explained by seven fragments of a comet that impacted the ocean at seven locations on Earth at 03.00h (C.E.T.) on 23 September, 9545 yr BP. We demonstrate that all the ‘geological proofs’ that allegedly support their conclusions are not supported by the available data on impact cratering. Their hypothesis is based on insufficient and ambiguous data, selective citation, and incomplete comprehension of previous research. 相似文献
84.
85.
86.
J. Crummy A. C. Fabian L. Gallo R. R. Ross 《Monthly notices of the Royal Astronomical Society》2006,365(4):1067-1081
We present a large sample of type 1 active galactic nuclei (AGN) spectra taken with XMM–Newton , and fit them with both the conventional model (a power law and blackbody) and the relativistically blurred photoionized disc reflection model of Ross & Fabian. We find that the disc reflection model is a better fit. The disc reflection model successfully reproduces the continuum shape, including the soft excess, of all the sources. The model also reproduces many features that would conventionally be interpreted as absorption edges. We are able to use the model to infer the properties of the sources, specifically that the majority of black holes in the sample are strongly rotating, and that there is a deficit in sources with an inclination >70°. We conclude that the disc reflection model is an important tool in the study of AGN X-ray spectra. 相似文献
87.
88.
On the X-ray spectra of luminous, inhomogeneous accretion flows 总被引:1,自引:0,他引:1
A. Merloni J. Malzac A. C. Fabian R. R. Ross 《Monthly notices of the Royal Astronomical Society》2006,370(4):1699-1712
89.
90.
Matt J. Jarvis Ross J. McLure 《Monthly notices of the Royal Astronomical Society》2006,369(1):182-188
We have identified two new galaxies with gas counter-rotation (NGC 1596 and 3203) and have confirmed similar behaviour in another one (NGC 128), this using results from separate studies of the ionized-gas and stellar kinematics of a well-defined sample of 30 edge-on disc galaxies. Gas counter-rotators thus represent 10 ± 5 per cent of our sample, but the fraction climbs to 21 ± 11 per cent when only lenticular (S0) galaxies are considered and to 27 ± 13 per cent for S0 galaxies with detected ionized gas only. Those fractions are consistent with but slightly higher than previous studies. A compilation from well-defined studies of S0 galaxies in the literature yields fractions of 15 ± 4 and 23 ± 5 per cent, respectively. Although mainly based on circumstantial evidence, we argue that the counter-rotating gas originates primarily from minor mergers and tidally induced transfer of material from nearby objects. Assuming isotropic accretion, twice those fractions of objects must have undergone similar processes, underlining the importance of (minor) accretion for galaxy evolution. Applications of gas counter-rotators to barred galaxy dynamics are also discussed. 相似文献