全文获取类型
收费全文 | 84篇 |
免费 | 1篇 |
国内免费 | 2篇 |
专业分类
测绘学 | 1篇 |
地球物理 | 8篇 |
地质学 | 24篇 |
天文学 | 50篇 |
自然地理 | 4篇 |
出版年
2021年 | 1篇 |
2020年 | 2篇 |
2018年 | 5篇 |
2017年 | 3篇 |
2016年 | 5篇 |
2015年 | 1篇 |
2014年 | 4篇 |
2013年 | 3篇 |
2012年 | 1篇 |
2011年 | 6篇 |
2009年 | 9篇 |
2008年 | 2篇 |
2007年 | 4篇 |
2006年 | 7篇 |
2005年 | 2篇 |
2004年 | 4篇 |
2003年 | 4篇 |
2001年 | 4篇 |
2000年 | 2篇 |
1999年 | 3篇 |
1998年 | 3篇 |
1994年 | 1篇 |
1990年 | 1篇 |
1989年 | 2篇 |
1987年 | 1篇 |
1986年 | 1篇 |
1985年 | 1篇 |
1984年 | 2篇 |
1982年 | 2篇 |
1981年 | 1篇 |
排序方式: 共有87条查询结果,搜索用时 15 毫秒
11.
12.
M. Jamrozy C. Konar D. J. Saikia . Stawarz K.-H. Mack A. Siemiginowska 《Monthly notices of the Royal Astronomical Society》2007,378(2):581-593
We present radio observations at frequencies ranging from 240 to 8460 MHz of the radio galaxy 4C 29.30 (J0840+2949) using the Giant Metrewave Radio Telescope (GMRT), the Very Large Array (VLA) and the Effelsberg telescope. We report the existence of weak extended emission with an angular size of ∼520 arcsec (639 kpc) within which a compact edge-brightened double-lobed source with a size of 29 arcsec (36 kpc) is embedded. We determine the spectrum of the inner double from 240 to 8460 MHz and show that it has a single power-law spectrum with a spectral index of ∼0.8. Its spectral age is estimated to be ≲33 Myr. The extended diffuse emission has a steep spectrum with a spectral index of ∼1.3 and a break frequency ≲240 MHz. The spectral age is ≳200 Myr, suggesting that the extended diffuse emission is due to an earlier cycle of activity. We re-analyse archival X-ray data from Chandra and suggest that the X-ray emission from the hotspots consists of a mixture of non-thermal and thermal components, the latter being possibly due to gas which is shock heated by the jets from the host galaxy. 相似文献
13.
Saikia D. J. Shastri P. Cornwell T. J. Junor W. Muxlow T. W. B. 《Journal of Astrophysics and Astronomy》1989,10(2):203-235
As part of our study to understand the nature of extragalactic radio sources which are very asymmetric in the surface brightness
of the two lobes, often with radio emission on only one side of the nucleus, we have observed a large number of them with
high angular resolution and good surface brightness sensitivity at radio frequencies. In this paper we present VLA and MERLIN
observations of 15 such sources. We discuss their observed structures and spectra, and possible explanations for their morphologies.
We report evidence of a possible correlation between the hot-spot brightness ratio and the degree of core prominence, used
as a Statistical measure of source orientation, suggesting that relativistic beaming of the hot-spot emission does play a
significant role in the observed brightness asymmetry. To explain the apparently one-sided sources within the relativistic
beaming framework, the velocities required are in the range of 0.2 to 0.8c. We discuss the possibility that the lobe which is seen to the south of the jet in 3C273 is the counter-lobe seen in projection.
We also draw-attention to a number of one-sided sources with very weak cores, and discuss their possible nature. 相似文献
14.
We have reinvestigated the reported tendency for the extended radio structures associated with bright elliptical galaxies
to be oriented preferentially along the optical minor axes. It is found that such a tendency exists only for those galaxies
in which the compact radio cores coincident with their nuclei are quite prominent. If the galaxies are divided into two groups
according to whether their cores account for less than or greater than 10 per cent of the total flux density at 2.7 GHz, the
angle Φ (between the radio axis and the optical minor axis) appears to be uniformly distributed between 0‡ and 90‡ for the
former, but is nearly always < 30‡ for the latter group. One possible explanation is that the radio emission from compact
cores suffers thermal absorption by ionized gas that is distributed differently in the two groups. 相似文献
15.
Using a large sample of 78 well-observed double quasars, we have investigated several consequences of the relativistic beaming
model. In this model the ratio of the strengths of the central component and outer lobes of a double source depends on whether
the jet axis lies close to or away from the line of sight, If this is the actual situation, the fraction of emission from
the core,f
c, may be used as a statistical measure of the orientation of the source and should be correlated with other source parameters
which also depend on the inclination of the jet axis to the line of sight.
We findf
c to be anticorrelated with the overall projected linear size of the extended emission but to exhibit a positive correlation
with both the observed degree of misalignment from a collinear double structure, and the ratio of separations of the outer
hotspots from the central component. As might be expected from these relationships, we also find sources of smaller projected
linear sizes to appear more misaligned and the degree of misalignment to be correlated with the ratio of separations of the
outer hotspots. All these correlations are consistent with the predictions of the relativistic beaming model. 相似文献
16.
Sagar Godambe C. Konar D. J. Saikia Paul J. Wiita 《Monthly notices of the Royal Astronomical Society》2009,396(2):860-869
We present low-frequency observations with the Giant Metrewave Radio Telescope of three giant radio sources (GRSs: J0139+3957, J0200+4049 and J0807+7400) with relaxed diffuse lobes which show no hotspots and no evidence of jets. The largest of these three, J0200+4049, exhibits a depression in the centre of the western lobe, while J0139+3957 and J0807+7400 have been suggested earlier by Klein et al. and Lara et al., respectively, to be relic radio sources. We estimate the ages of the lobes. We also present Very Large Array observations of the core of J0807+7400, and determine the core radio spectra for all three sources. Although the radio cores suggest that the sources are currently active, we explore the possibility that the lobes in these sources are due to an earlier cycle of activity. 相似文献
17.
Binoy K. Saikia 《Journal of the Geological Society of India》2009,74(6):749-752
An examination on the structural features of some coal samples from Makum coalfield, Assam (India) were carried out by using
scanning electron microscopy. The morphological characteristics of the macerals were recognized. Collinite was recognizable
by its angular shape with characteristic fracture patterns and striated or laminated surfaces. Sporinite particles showed
no well-defined shape. Fusinite was remarkable in having a chunky needle form. Chemical and petrographic characteristics of
these coals also have been reported. These findings have shown prime importance in fingerprinting the physical structure of
these coals. 相似文献
18.
19.
A. Pirya S. Nandi D. J. Saikia C. Konar M. Singh 《Journal of Astrophysics and Astronomy》2011,32(4):471-474
We present the results of GMRT and VLA observations of five large radio sources over a wide frequency range to investigate
their structural and spectral asymmetries. The hot-spot brightness ratios suggest intrinsic source asymmetries, while the
spectral indices show evidence of re-acceleration of particles. 相似文献
20.
Binoy K. Saikia Arpita Sharma Kakoli Khound Bimala P. Baruah 《Journal of the Geological Society of India》2013,82(3):295-298
Five representative sub-bituminous coals from NE part of India have been analyzed with respect to their distribution of carbon functional groups through 13C solid state NMR experiments. The 13C Cross Polarised/Magic Angle Spinning NMR spectra of the coal samples were recorded at temperatures of 23°C, 50°C and 70°C respectively and the changes on their structures were interpreted. The NMR spectra of low rank coals were found to exhibit varying degrees of fine structures. The aromaticities of the coal were also determined from the C/H ratios of coal. Some changes in the peak positions along with the formation of simple aromatic units were observed on mild heating. 相似文献