Geochemical and oxygen isotope perspective of a new R chondrite Dhofar 1671: Affinity with ordinary chondrites          下载免费PDF全文

Arshad Ali  Sobhi J. Nasir  Iffat Jabeen  Ahmed Al Rawas  Neil R. Banerjee  Gordon R. Osinski 《Meteoritics & planetary science》2017,52(9):1991-2003

Dhofar 1671 is a relatively new meteorite that previous studies suggest belongs to the Rumuruti chondrite class. Major and REE compositions are generally in agreement with average values of the R chondrites (RCs). Moderately volatile elements such as Se and Zn abundances are lower than the R chondrite values that are similar to those in ordinary chondrites (OCs). Porphyritic olivine pyroxene (POP), radial pyroxene (RP), and barred olivine (BO) chondrules are embedded in a proportionately equal volume of matrix, one of the characteristic features of RCs. Microprobe analyses demonstrate compositional zoning in chondrule and matrix olivines showing Fa‐poor interior and Fa‐rich outer zones. Precise oxygen isotope data for chondrules and matrix obtained by laser‐assisted fluorination show a genetic isotopic relationship between OCs and RCs. On the basis of our data, we propose a strong affinity between these groups and suggest that OC chondrule precursors could have interacted with a ¹⁷O‐rich matrix to form RC chondrules (i.e., ?¹⁷O shifts from ~1‰ to ~3‰). These interactions could have occurred at the same time as “exotic” clasts in brecciated samples formed such as NWA 10214 (LL3–6), Parnallee (LL3), PCA91241 (R3.8–6), and Dhofar 1671 (R3.6). We also infer that the source of the oxidation and ¹⁷O enrichment is the matrix, which may have been enriched in ¹⁷O‐rich water. The abundance of matrix in RCs relative to OCs, ensured that these rocks would be apparently more oxidized and appreciably ¹⁷O‐enriched. In situ analysis of Dhofar 1671 is recommended to further strengthen the link between OCs and RCs.  相似文献   

Static cylindrically symmetric gravitational field with cosmological constant     

A. Banerjee  Antares Kleber  Nilton O. Santos 《Astrophysics and Space Science》1996,245(1):139-149

We show that a class of solutions for a vacuum cylindrically symmetric gravitational field with nonvanishing cosmological constant reduce to the welknown Levi-Civita metric close to the axis. All the circular geodesics in this generalized vacuum are time like, null or space like depending on the relative magnitudes of the two parameters appearing in the solutions.For other particles moving inZ=constant plane there are some cases where the trapping of timelike and null trajectories occur, while in other cases some of the particles may orbit round the axis in a fixed zone bounded by two limiting radii.  相似文献   

Exact solutions in (2+1)-dimensional anti-de Sitter space-time admitting a linear or non-linear equation of state     

Ayan Banerjee  Farook Rahaman  Kanti Jotania  Ranjan Sharma  Mosiur Rahaman 《Astrophysics and Space Science》2015,355(2):353-359

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Collisional hardening of compact binaries in globular clusters     

S. Banerjee  P. Ghosh 《Monthly notices of the Royal Astronomical Society》2006,373(3):1188-1194

We consider essential mechanisms for orbit shrinkage or 'hardening' of compact binaries in globular clusters (GCs) to the point of Roche lobe contact and X-ray emission phase, focusing on the process of collisional hardening due to encounters between binaries and single stars in the cluster core. The interplay between this kind of hardening and that due to emission of gravitational radiation produces a characteristic scaling of the orbit-shrinkage time with the single-star binary encounter rate γ in the cluster which we introduce, clarify and explore. We investigate possible effects of this scaling on populations of X-ray binaries in GCs within the framework of a simple 'toy' scheme for describing the evolution of pre-X-ray binaries in GCs. We find the expected qualitative trends sufficiently supported by data on X-ray binaries in Galactic GCs to encourage us towards a more quantitative study.  相似文献   

On searches for gravitational waves from mini-creation events by laser interferometric detectors     

B. P. Sarmah  S. K. Banerjee  S. V. Dhurandhar  J. V. Narlikar 《Monthly notices of the Royal Astronomical Society》2006,369(1):89-96

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Supersonic turbulence, filamentary accretion and the rapid assembly of massive stars and discs     

Robi Banerjee  Ralph E. Pudritz  Dave W. Anderson 《Monthly notices of the Royal Astronomical Society》2006,373(3):1091-1106

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Critical properties and stability of stationary solutions in multitransonic pseudo-Schwarzschild accretion     

Soumini Chaudhury  Arnab K. Ray  Tapas K. Das 《Monthly notices of the Royal Astronomical Society》2006,373(1):146-156

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Anisotropic viscous-fluid cosmological model     

A. Banerjee  M. B. Ribeiro  N. O. Santos 《Astrophysics and Space Science》1987,136(2):331-336

We present exact solutions of a Bianchi type VI₀ viscous fluid cosmological model. It is a generalization of the model proposed by Banerjee and Santos (1983) for Bianchi type I.  相似文献   

Diffusion coefficient of neutrinos in a pre-supernova star     

B. Banerjee  S. M. Chitre  Namrata Rajeev 《Astrophysics and Space Science》1993,205(2):343-353

The diffusion coefficient of neutrinos in the trapping regime in a presupernova star,where the scattering of neutrinos by nuclei is the dominant effect, is calculated within the framework of relativistic kinetic theory in the lowest order Chapman-Enskog approximation. The screening of the nuclei by ion-ion and electron-electron correlations is also taken into account.  相似文献   

Petrographic observations suggestive of microbial mats from Rampur Shale and Bijaigarh Shale, Vindhyan basin, India     

S. Sur  J. Schieber  S. Banerjee 《Journal of Earth System Science》2006,115(1):61-66

Petrographic observations of two Vindhyan black shales (Rampur Shale of the Semri Group and Bijaigarh Shale of the Kaimur Group) revealed the following features:

–	•general wavy lamination,
–	•contorted and folded thin shreds of organic matter,
–	•wavy pyritic laminae,
–	•‘teeth and socket’ structure.

These features are indirect evidence of microbial mat colonization during the Proterozoic. The microbial mats probably fixed carbon at the sediment surface, stabilized sediment and recycled organic matter and were the primary producers, unlike during the Phanerozoic time.  相似文献