排序方式： 共有10条查询结果，搜索用时 984 毫秒
1
1.
Kepler SO Mukadam A Winget DE Nather RE Metcalfe TS Reed MD Kawaler SD Bradley PA 《The Astrophysical journal》2000,534(2):L185-L188
We observe G117-B15A, the most precise optical clock known, to measure the rate of change of the main pulsation period of this blue-edge DAV white dwarf. Even though the obtained value is only within 1 sigma, P&d2;=&parl0;2.3+/-1.4&parr0;x10-15 s s-1, it is already constraining the evolutionary timescale of this cooling white dwarf star. 相似文献
2.
3.
D. W.Kurtz S. D.Kawaler R. L.Riddle M. D.Reed † M. S.Cunha M.Wood N.Silvestri T. K.Watson N.Dolez P.Moskalik S.Zola E.Pallier J. A.Guzik T. S.Metcalfe A. S.Mukadam R. E.Nather D. E.Winget D. J.Sullivan T.Sullivan K.Sekiguchi X.Jiang R.Shobbrook B. N.Ashoka S.Seetha S.Joshi D.O'Donoghue G.Handler M.Mueller J. M.Gonzalez Perez J.-E.Solheim F.Johannessen A.Ulla S. O.Kepler A.Kanaan A.da Costa L.Fraga O.Giovannini J. M.Matthews 《Monthly notices of the Royal Astronomical Society》2002,330(3):57-61
HR 1217 is a prototypical rapidly oscillating Ap star that has presented a test to the theory of non-radial stellar pulsation. Prior observations showed a clear pattern of five modes with alternating frequency spacings of 33.3 and 34.6 μHz, with a sixth mode at a problematic spacing of 50.0 μHz (which equals 1.5×33.3 μHz) to the high-frequency side. Asymptotic pulsation theory allowed for a frequency spacing of 34 μHz, but Hipparcos observations rule out such a spacing. Theoretical calculations of magnetoacoustic modes in Ap stars by Cunha predicted that there should be a previously undetected mode 34 μHz higher than the main group, with a smaller spacing between it and the highest one. In this Letter, we present preliminary results from a multisite photometric campaign on the rapidly oscillating Ap star HR 1217 using the 'Whole Earth Telescope'. While a complete analysis of the data will appear in a later paper, one outstanding result from this run is the discovery of a newly detected frequency in the pulsation spectrum of this star, at the frequency predicted by Cunha. 相似文献
4.
Qian JianxingThe Second Institute of Oceanography SO A Hangzhuu Zhejiang Liu Linqun 《《地质学报》英文版》1995,69(2)
Based on a comparison between the oxygen isotope records of benthic and plank tonic foraminifers from core 8KL of the South China Sea and sea-level change records derived from the Huon Peninsula, New Guinea, it is found that both records are very similar from 72 K a B.P. to the present, especially for the benthic oxygen isotope record. The linear regression shows that δ18O changes (0.9995‰ for benthic foraminifers and 1.022‰ for planktonic foraminifers) are equal to 100 m in sea-level fluctuation. After making temperature correction in the δ18O record of benthic foraminifers from 72 to 120 Ka B.P., the curve of sea-level oscillation of the South China Sea since 186 Ka B.P. has been reconstructed. The lowermost sea - level that occurred in the last glacial maximum and oxygen isotope stage 6 is approximately - 130 m. 相似文献
5.
6.
B. G. Castanheira S. O. Kepler 《Monthly notices of the Royal Astronomical Society》2009,396(3):1709-1731
We used the detected pulsation modes and adiabatic pulsation models to do seismology of the class of ZZ Ceti stars and measure the H layer mass for 83 stars. We found the surface hydrogen layer to be within the range 10−9.5 ≥ M H / M * ≥ 10−4 , with an average of M H / M * = 10−6.3 , which is thinner than the predicted value of M H / M * = 10−4 , indicating that the stars lose more mass during their evolution than previously expected. These results are preliminary and do not include the possible effects of realistic C/O profiles on the fits. 相似文献
7.
The Sinuiju Formation in Paekto-dong, Sinuiju City in the Democratic People's Republic of Korea has yielded Mesozoic nonmarine bivalve fossils, which is the first occurrence of such in the DPRK. Based on these fossil specimens, a new Cretaceous bivalve assemblage, the Arguniella yanshanensis-Sphaerium anderssoni Assemblage is erected. This assemblage includes Arguniella yanshanensis, A. lingyuanensis and Sphaerium anderssoni and can be compared with the Jehol Biota. The age of the Sinuiju Formation is also clarified and on the basis of the bivalves and the presence of a Eosestheria–Ephemeropsis–Lycoptera(E–E–L) assemblage, the formation is not Upper Jurassic, but Lower Cretaceous in age. 相似文献
8.
B. Pfeiffer G. Vauclair N. Dolez M. Chevreton J. R. Fremy G. Herpe M. Barstow S. J. Kleinman T. K. Watson J. A. Belmonte S. O Kepler A. Kanaan O. Giovannini R. E. Nather D. E. Winget J. Provencal J. C. Clemens P. Bradley J. Dixson A. D. Grauer G. Fontaine P. Bergeron F. Wesemael C. F. Claver T. Matzeh E. Leibowitz P. Moskalik 《Astrophysics and Space Science》1993,210(1-2):201-204
9.
Seong–Taek YUN Seung–Jun YOUM Chil–Sup SO Seon–Gyu CHOI De–Quan ZHANG Yong–Kwon KOH 《Resource Geology》2001,51(3):205-215
Abstract: Gold mineralization of the Daerae mine represents the first recognized example of the Jurassic gold mineralization in the Sangju area, Korea. It occurs as a single stage of quartz veins that fill fault fractures in Precambrian gneiss of the central‐northern Sobaegsan Massif. The mineralogical characteristics of quartz veins, such as the simple mineralogy and relatively gold‐rich (65–72 atomic % Au) nature of electrum, as well as the CO2–rich and low salinity nature of fluid inclusions, are consistent with the ‘mesothermal‐type’ gold deposits previously recognized in the Youngdong area (about 50 km southwest of the Sangju area). Ore fluids were evolved mainly through CO2 immiscibility at temperatures between about 250 and 325 C. Vein sulfides characteristically have negative sulfur isotopic values (–1.9 to +0.2 %), which have been very rarely reported in South Korea, and possibly indicate the derivation of sulfur from an ilmenite‐series granite melt. The calculated O and H isotopic compositions of hydrothermal fluids at Daerae (δ18Owater = +5.2 to +5.9 %; δDwater = –59 to –67 %) are very similar to those from the Youngdong area, and indicate the important role of magmatic water in gold mineralization. The 40Ar–39Ar age dating of a pure alteration sericite sample yields a high‐temperature plateau age of 188.3 0.1 Ma, indicating an early Jurassic age for the gold mineralization at Daerae. The lower temperature Ar‐Ar plateau defines an age of 158.4 2.0 Ma (middle Jurassic), interpreted as reset by a subsequent thermal effect after quartz vein formation. The younger plateau age is the same as the previously reported K‐Ar ages (145–171 Ma) for the other ‘mesothermal–type’ gold deposits in the Youngdong and Jungwon areas, Korea, which are too young in view of the new Jurassic Ar‐Ar plateau age (around 188 Ma). 相似文献
10.
D. J. Sullivan † T. S. Metcalfe D. O'Donoghue D. E. Winget D. Kilkenny F. van Wyk A. Kanaan S. O. Kepler A. Nitta S. D. Kawaler M. H. Montgomery R. E. Nather M. S. O'Brien A. Bischoff-Kim M. Wood X. J. Jiang E. M. Leibowitz P. Ibbetson S. Zola J. Krzesinski G. Pajdosz G. Vauclair N. Dolez M. Chevreton 《Monthly notices of the Royal Astronomical Society》2008,387(1):137-152
1