Historical optical data are combined on the BL Lac object OQ 530. Verifying the existence of correlations among the flux variations in different bands serves as an important tool to investigate emission processes. To ...Historical optical data are combined on the BL Lac object OQ 530. Verifying the existence of correlations among the flux variations in different bands serves as an important tool to investigate emission processes. To examine the possible existence of a lag between variations in different optical bands from this source, a statistical analysis is performed through the discrete correlation function （DCF） method and the z-transformed discrete correlation function （ZDCF） method. Monte Carlo simulations called ＂flux redistribution/random subset selection＂ （FR/RSS） are performed to obtain statistically meaningful values for the cross-correlation time lags and their related uncertainties. The analysis confirms that the variations in different optical light curves are strongly correlated, with zero-lag within the errors. Long term variability of color indexes is also analyzed. The result suggests a strong correlation between color index and brightness. A clear bluer-when-brighter chromatism is found, in the sense that the spectrum steepens as the brightness decreases.展开更多
The post-1994 observations of the blazar OQ 530 in optical BVRI bands, and radio observations at 22 GHz and 37 GHz were collected. The date compensated discrete Fourier transform （DCDFr） and CLEANest methods were us...The post-1994 observations of the blazar OQ 530 in optical BVRI bands, and radio observations at 22 GHz and 37 GHz were collected. The date compensated discrete Fourier transform （DCDFr） and CLEANest methods were used to search for possible periodicities. Two possible periods of 456±100 days and 258±29 days were found in the optical bands. The existence of possible correlations between the optical and radio emissions was investigated by means of discrete correlation function （DCF） analysis, and no significant correlation was found. Some possible mechanisms for the periodic variability are discussed.展开更多
We present the results of VLBI observations at 5 GHz and 8.4 GHz of the compact symmetric object (CSO) OQ208. Images taken on four epochs at 5GHz and one at 8.4GHz show that the parsec radio structure of the source co...We present the results of VLBI observations at 5 GHz and 8.4 GHz of the compact symmetric object (CSO) OQ208. Images taken on four epochs at 5GHz and one at 8.4GHz show that the parsec radio structure of the source consists of two mini-lobes, both of them are resolved into two hot-spots. We note that the component D is stronger than the component C in the south-west region at 5 GHz, indicating that component D is less free-free absorbed than C at low frequency. On the basis of the separation of components A and D, a proper motion of 0.032±0.02 mas yrbetween the two mini-lobes is estimated. This value is about half the previous estimates based on the separation of components A and C with 8.4 GHz VLBI data. The reason for the decrease in the expansion velocity is discussed.展开更多
We report on an ongoing work aimed to detect the separation speed of the two hot-spots of the compact symmetric object OQ208.Comparing images at 8.4 GHz taken in 6 epoches between 1994 and 1997 we obtain an estimate o...We report on an ongoing work aimed to detect the separation speed of the two hot-spots of the compact symmetric object OQ208.Comparing images at 8.4 GHz taken in 6 epoches between 1994 and 1997 we obtain an estimate of 0.058±-0.038 mas/year as the relative motions between two components of the radio source.At the red-shift of OQ208 I mas correspond to 1pc,thus we obtain a projected jet speed of 0.095±0.062c.With an inclination of 45°between the jets and the line of sight,we have an actual jet velocity of 0.134±0.088c and therefore the kinematic age of the source is so young of 320±210 years.展开更多
The first charge-coupled device photometric light curves in B,V,Rc,and Ic bands of the short-period contact binary star OQ Cam are presented.Through analyzing the light curves with the WilsonDevinney code,it is found ...The first charge-coupled device photometric light curves in B,V,Rc,and Ic bands of the short-period contact binary star OQ Cam are presented.Through analyzing the light curves with the WilsonDevinney code,it is found that OQ Cam is a W-type shallow contact binary star with a contact degree of f=20.2%.Based on the O-C analyzing,the orbit period displays a long term increasing with a rate of d P/dt=4.40×10^-7 d yr-1.The increasing in orbit period can be interpreted by mass transfer from the less massive component to the more massive one.As the orbit period increases,OQ Cam would evolve from the present shallow contact configuration to a non-contact stage.So it may be a potential candidate to confirm the thermal relaxation oscillation theory.展开更多
We present quasi-simultaneous VLBI images of the GHz-Peaked-Spectrum radio source OQ 208 obtained with the Very Long Baseline Array at 1.4, 1.7, 2.3, 5.0, 8.4, 15.4 GHz and the European VLBI Network at 6.7 GHz. The lo...We present quasi-simultaneous VLBI images of the GHz-Peaked-Spectrum radio source OQ 208 obtained with the Very Long Baseline Array at 1.4, 1.7, 2.3, 5.0, 8.4, 15.4 GHz and the European VLBI Network at 6.7 GHz. The low frequency （1.4, 1.7 and 2.3 GHz） observations reveal a weak and extended steep-spectrum component at about 30 mas away at position angle - 110°, which may be a remnant emission. The radio structure of OQ 208 consists of two mini-lobes at 5.0, 6.7, 8.4 and 15.4 GHz. Our spectral analysis further confirms that the southwest lobe undergoes free-free absorption and finds that the free-free absorption is stronger in the inner region. By fitting the 8.4 GHz images from 1994 to 2005, we obtain a separation speed of 0.0314-0.006 mas yr^-1 between the two mini-lobes. This indicates a jet proper motion of 0.1054-0.020 c and a kinematic age of 219±42 yr for the radio source.展开更多
淬火-配分(Quenching and Partitioning,Q&P)钢由于具有优异的综合性能而备受关注。本文设计了一步等温和二步等温处理工艺,通过改变淬火温度和等温温度获得了不同含量一次马氏体(PM)、残余奥氏体(RA)、二次马氏体(FM)及贝氏体(BF)...淬火-配分(Quenching and Partitioning,Q&P)钢由于具有优异的综合性能而备受关注。本文设计了一步等温和二步等温处理工艺,通过改变淬火温度和等温温度获得了不同含量一次马氏体(PM)、残余奥氏体(RA)、二次马氏体(FM)及贝氏体(BF)的多相微观结构。采用XRD、EBSD综合分析了淬火配分处理对马氏体/贝氏体形态、位错密度、体积含量、变体选择行为以及冲击韧性的影响。示波冲击试验结果表明:330℃是一步淬火配分和二步淬火配分处理的最佳淬火温度,该温度能够获得最佳的冲击韧性。与一步淬火配分处理比较,二步淬火配分处理可以提高复相组织中的RA含量,并降低FM含量。最优的淬火温度和配分温度有利于降低马氏体/贝氏体(M/B)中的位错密度、增加RA和大角度晶界(HAGB)体积含量,从而显著改善Q&P钢的冲击韧性。展开更多
基金Supported by the National Natural Science Foundation of China (Grant No. 10975145)funded by Fuyang Normal College, the Research Foundation of the Department of Education of Anhui Province (KJ2010B159)
文摘Historical optical data are combined on the BL Lac object OQ 530. Verifying the existence of correlations among the flux variations in different bands serves as an important tool to investigate emission processes. To examine the possible existence of a lag between variations in different optical bands from this source, a statistical analysis is performed through the discrete correlation function （DCF） method and the z-transformed discrete correlation function （ZDCF） method. Monte Carlo simulations called ＂flux redistribution/random subset selection＂ （FR/RSS） are performed to obtain statistically meaningful values for the cross-correlation time lags and their related uncertainties. The analysis confirms that the variations in different optical light curves are strongly correlated, with zero-lag within the errors. Long term variability of color indexes is also analyzed. The result suggests a strong correlation between color index and brightness. A clear bluer-when-brighter chromatism is found, in the sense that the spectrum steepens as the brightness decreases.
基金the National Natural Science Foundation of China
文摘The post-1994 observations of the blazar OQ 530 in optical BVRI bands, and radio observations at 22 GHz and 37 GHz were collected. The date compensated discrete Fourier transform （DCDFr） and CLEANest methods were used to search for possible periodicities. Two possible periods of 456±100 days and 258±29 days were found in the optical bands. The existence of possible correlations between the optical and radio emissions was investigated by means of discrete correlation function （DCF） analysis, and no significant correlation was found. Some possible mechanisms for the periodic variability are discussed.
基金Supported by the National Natural Science Foundation of China
文摘We present the results of VLBI observations at 5 GHz and 8.4 GHz of the compact symmetric object (CSO) OQ208. Images taken on four epochs at 5GHz and one at 8.4GHz show that the parsec radio structure of the source consists of two mini-lobes, both of them are resolved into two hot-spots. We note that the component D is stronger than the component C in the south-west region at 5 GHz, indicating that component D is less free-free absorbed than C at low frequency. On the basis of the separation of components A and D, a proper motion of 0.032±0.02 mas yrbetween the two mini-lobes is estimated. This value is about half the previous estimates based on the separation of components A and C with 8.4 GHz VLBI data. The reason for the decrease in the expansion velocity is discussed.
基金Supported by the 95 Basic Research Key Project of Chinese Academy of Sciences under Grant No.KJ952-J303.
文摘We report on an ongoing work aimed to detect the separation speed of the two hot-spots of the compact symmetric object OQ208.Comparing images at 8.4 GHz taken in 6 epoches between 1994 and 1997 we obtain an estimate of 0.058±-0.038 mas/year as the relative motions between two components of the radio source.At the red-shift of OQ208 I mas correspond to 1pc,thus we obtain a projected jet speed of 0.095±0.062c.With an inclination of 45°between the jets and the line of sight,we have an actual jet velocity of 0.134±0.088c and therefore the kinematic age of the source is so young of 320±210 years.
基金supported by National Natural Science Foundation of China (NSFC) (No. 11703016)by the Joint Research Fund in Astronomy (Nos. U1631108 and U1931103) under cooperative agreement between NSFC and Chinese Academy of Sciences (CAS)+4 种基金by the Natural Science Foundation of Shandong Province (Nos. ZR2014AQ019, ZR2017PA009, ZR2017PA010 and JQ201702)by Young Scholars Program of Shandong University, Weihai (Nos. 20820162003 and 20820171006)by the Chinese Academy of Sciences Interdisciplinary Innovation Teamby the Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects (No. OP201704)partly supported by the Supercomputing Center of Shandong University, Weihai.
文摘The first charge-coupled device photometric light curves in B,V,Rc,and Ic bands of the short-period contact binary star OQ Cam are presented.Through analyzing the light curves with the WilsonDevinney code,it is found that OQ Cam is a W-type shallow contact binary star with a contact degree of f=20.2%.Based on the O-C analyzing,the orbit period displays a long term increasing with a rate of d P/dt=4.40×10^-7 d yr-1.The increasing in orbit period can be interpreted by mass transfer from the less massive component to the more massive one.As the orbit period increases,OQ Cam would evolve from the present shallow contact configuration to a non-contact stage.So it may be a potential candidate to confirm the thermal relaxation oscillation theory.
基金Supported by the National Natural Science Foundation of China.
文摘We present quasi-simultaneous VLBI images of the GHz-Peaked-Spectrum radio source OQ 208 obtained with the Very Long Baseline Array at 1.4, 1.7, 2.3, 5.0, 8.4, 15.4 GHz and the European VLBI Network at 6.7 GHz. The low frequency （1.4, 1.7 and 2.3 GHz） observations reveal a weak and extended steep-spectrum component at about 30 mas away at position angle - 110°, which may be a remnant emission. The radio structure of OQ 208 consists of two mini-lobes at 5.0, 6.7, 8.4 and 15.4 GHz. Our spectral analysis further confirms that the southwest lobe undergoes free-free absorption and finds that the free-free absorption is stronger in the inner region. By fitting the 8.4 GHz images from 1994 to 2005, we obtain a separation speed of 0.0314-0.006 mas yr^-1 between the two mini-lobes. This indicates a jet proper motion of 0.1054-0.020 c and a kinematic age of 219±42 yr for the radio source.
文摘淬火-配分(Quenching and Partitioning,Q&P)钢由于具有优异的综合性能而备受关注。本文设计了一步等温和二步等温处理工艺,通过改变淬火温度和等温温度获得了不同含量一次马氏体(PM)、残余奥氏体(RA)、二次马氏体(FM)及贝氏体(BF)的多相微观结构。采用XRD、EBSD综合分析了淬火配分处理对马氏体/贝氏体形态、位错密度、体积含量、变体选择行为以及冲击韧性的影响。示波冲击试验结果表明:330℃是一步淬火配分和二步淬火配分处理的最佳淬火温度,该温度能够获得最佳的冲击韧性。与一步淬火配分处理比较,二步淬火配分处理可以提高复相组织中的RA含量,并降低FM含量。最优的淬火温度和配分温度有利于降低马氏体/贝氏体(M/B)中的位错密度、增加RA和大角度晶界(HAGB)体积含量,从而显著改善Q&P钢的冲击韧性。
