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11.
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
12.
Turatto M Suzuki T Mazzali PA Benetti S Cappellaro E Danziger IJ Nomoto K Nakamura T Young TR Patat F 《The Astrophysical journal》2000,534(1):L57-L61
The extraordinary SN 1997cy associated with GRB 970514 has been observed photometrically and spectroscopically for nearly 2 yr. At the time of discovery, SN 1997cy was the brightest supernova (SN) ever observed (MV=-20.1, vhel=19,140 km s-1, H0=65 km s-1 Mpc-1). Up to the last available observations (600 days after the gamma-ray burst), the total time-integrated flux was equal to or larger than that expected from the complete thermalization of the gamma-rays produced by 2.3 M middle dot in circle of 56Co. However, starting already on day 60 the luminosity decline is slower than the 56Co decay rate, indicating that the SN ejecta was interacting with circumstellar material (CSM). The interaction appeared to weaken around day 550. The spectra of SN 1997cy are dominated at all epochs by Halpha emission, which shows at least three components of different widths, as in SN 1988Z. Several other lines with different widths are also visible, especially at early epochs. The entire light curve of SN 1997cy is reproduced by a model of the interaction of the very energetic (E=3x1052 ergs) ejecta of a massive star (25 M middle dot in circle) with the CSM, with some contribution from radioactive decays. The CSM could have been ejected with a mass-loss rate of M&d2; approximately 4x10-4 M middle dot in circle yr-1 as the progenitor star evolved from a blue to a red supergiant about 104 yr before the explosion. The lack of oxygen and magnesium lines in the spectra at nebular phases poses a problem for models requiring high-mass progenitors. The possibility that most of the core material of the progenitor has fallen onto a massive black hole so that the reverse shock dies at the inner edge of the H/He envelope is discussed. 相似文献
13.
Melchiorri A Ade PA de Bernardis P Bock JJ Borrill J Boscaleri A Crill BP De Troia G Farese P Ferreira PG Ganga K de Gasperis G Giacometti M Hristov VV Jaffe AH Lange AE Masi S Mauskopf PD Miglio L Netterfield CB Pascale E Piacentini F Romeo G Ruhl JE Vittorio N 《The Astrophysical journal》2000,536(2):L63-L66
We use the angular power spectrum of the cosmic microwave background, measured during the North American test flight of the Boomerang experiment, to constrain the geometry of the universe. Within the class of cold dark matter models, we find that the overall fractional energy density of the universe Omega is constrained to be 0.85=Omega=1.25 at the 68% confidence level. Combined with the COBE measurement, the data on degree scales from the Microwave Anisotropy Telescope in Chile, and the high-redshift supernovae data, we obtain new constraints on the fractional matter density and the cosmological constant. 相似文献
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一引言中國東南部中生代末期花崗岩侵入體甚多,今日地質調查區域逐漸推廣,花崗岩之分佈亦逐渐明瞭,作者近年來在浙赣二省調查所得之經驗,證諸前人之研究及調查,覺花崗岩之分佈,亦非漫無規則,實與中國東南部之地質構造有莫大之關係焉。 相似文献
18.
Geomasking sensitive health data and privacy protection: an evaluation using an E911 database 总被引:2,自引:0,他引:2
Allshouse WB Fitch MK Hampton KH Gesink DC Doherty IA Leone PA Serre ML Miller WC 《国际地球制图》2010,25(6):443-452
Geomasking is used to provide privacy protection for individual address information while maintaining spatial resolution for mapping purposes. Donut geomasking and other random perturbation geomasking algorithms rely on the assumption of a homogeneously distributed population to calculate displacement distances, leading to possible under-protection of individuals when this condition is not met. Using household data from 2007, we evaluated the performance of donut geomasking in Orange County, North Carolina. We calculated the estimated k-anonymity for every household based on the assumption of uniform household distribution. We then determined the actual k-anonymity by revealing household locations contained in the county E911 database. Census block groups in mixed-use areas with high population distribution heterogeneity were the most likely to have privacy protection below selected criteria. For heterogeneous populations, we suggest tripling the minimum displacement area in the donut to protect privacy with a less than 1% error rate. 相似文献
19.
孙吴-嘉荫盆地嘉D1井孢粉地层学研究 总被引:3,自引:0,他引:3
对孙吴一嘉荫盆地北部逊克县的嘉DI井采集的孢粉和沟鞭藻类化石进行了分析研究,划分出?个特征较明显的孢粉组合:富饶组Betulaepollenires-Schizaeoisporites-Polypodiaceaesporites组合,总体反映晚白垩世晚期Maastrichtian期的特点;太平林场组Gothanipollis-Gabionisporis-Balmeisporites组合,时代为晚白垩世Santonian—Campanian期;淘淇河组上段Hammenia-Taxodiaceaepollenites-Appendicisportes组合,时代为早白垩Aptian—Albian期;淘淇河组下段Cicatricosporites-Cyathidites-Osmundacidites组合,时代为早白垩Valanginan—Barrcmian期。这是迄今该地区据钻井实际资料所发现的较连续孢粉组合序列。 相似文献
20.
根据十余口探井微体古生物分析结果和对多年来积累的大量微体古生物分析资料的复查 ,将东濮凹陷古近系沙河街三段 (ES3)和四段 (ES4 )的介形类化石群自下而上分为 3个组合和 3个亚组合 :Cyprinotus igneus组合 ,分布于沙四段下亚段 ;Cyprinotus altilis- Cyprinotus jiyangensis组合 ,分布于沙四段上亚段 ;H uabeinia sinensis组合 ,分布于沙三段 ,其中 H uabeinia obscura- H uabeinia costatispinata亚组合分布于沙三段下亚段 ,H uabeiniasinensis- Candona binxianensis亚组合分布于沙三段中亚段 ,H uabeinia huidongensis- Cyprinotus dongmingensis亚组合分布于沙三段上亚段。各化石组合特征比较清楚 ,为东濮凹陷沙三段、沙四段的划分以及与渤海沿岸盆地的对比提供了依据。虽然东濮凹陷缺少渤海沿岸盆地沙四段顶界的标志性化石 Austrocypris,但该区沙三段、沙四段介形类化石组合整体面貌与整个渤海沿岸盆地相比仍然具有可对比性 ,从介形类化石组合方面来确定本区沙三段、沙四段的界线仍然是可行的 相似文献