In this paper,we determine the photosphere evolution of PTF11rka which is a type Ic supernova (SN) by fitting its spectral energy distributions at different epochs.We find that the photosphere of PTF11rka expanded at ...In this paper,we determine the photosphere evolution of PTF11rka which is a type Ic supernova (SN) by fitting its spectral energy distributions at different epochs.We find that the photosphere of PTF11rka expanded at a constant velocity at early epochs,and the photosphere temperature increased slightly after reaching a minimum.These features are reminiscent of those of SN 2017dio.Based on the photosphere module that can describe the photosphere evolution of PTF11rka,we use the ^(56)Ni cascade decay model to fit its multiband light curves (LCs),finding that the model can well fit the photometric data.The derived ejecta mass and ^(56)Ni mass are respectively 8.76■ and 0.29-0.41■;the derived peak luminosity and the rise time of the theoretical bolometric LC of PTF11rka are ~8.24×10^(42)erg s^(-1) and ~35 days,respectively.Moreover,we find that the theoretical multiband LCs and the theoretical bolometric LC of PTF11rka do not show early-time excesses proposed in the literature.This indicates that additional energy sources (e.g.,the interaction between the ejecta and the circumstellar material)suggested to be responsible for the early-time excess can be neglected.展开更多
In this paper,we perform the detailed modeling for the light curves(LCs)of PTF 10iuv which is a calcium-rich(Ca-rich)supernova(SN)to constrain the physical properties of its ejecta and the energy sources,as well as th...In this paper,we perform the detailed modeling for the light curves(LCs)of PTF 10iuv which is a calcium-rich(Ca-rich)supernova(SN)to constrain the physical properties of its ejecta and the energy sources,as well as the explosion mechanism.We find that the^(56)Ni model and the56Ni plus circumstellar interaction model fail to explain the LCs,while the four-element(^(56)Ni,^(48)Cr,^(52)Fe,and^(44)Ti)model can account for the LCs.The ejecta mass of PTF10iuv derived by the model(1.52_(-0.25)^(+0.34)M_(⊙))is consistent with that of the merger of a sub-Chandrasekhar mass white dwarf.The early-time LCs were mainly powered by^(56)Ni whose mass is~0.03 M_(⊙),while the contributions of^(48)Cr and^(52)Fe can be neglected.The derived^(44)Ti mass(~0.25 M_(⊙))is~1.8 times the upper limit of the derived^(44)Ti mass of Ca-rich SN 2005E.We suggest that subtracting the contributions of the host-galaxy,which are unknown,and including the flux from other long-lived elements(e.g.,^(57)Co,^(55)Fe,^(60)Co)can reduce the amount of^(44)Ti,and that this value can be regarded as an upper limit.展开更多
目的探讨V1导联P波终末电势(P wave terminal force in lead V1,PtfV1)在心功能不全患者中的临床应用价值。方法 110例心功能不全患者及100例正常对照组纳入研究。测量、计算、记录所有入选者的体表心电图PtfV1数值,超声心动图左室射血...目的探讨V1导联P波终末电势(P wave terminal force in lead V1,PtfV1)在心功能不全患者中的临床应用价值。方法 110例心功能不全患者及100例正常对照组纳入研究。测量、计算、记录所有入选者的体表心电图PtfV1数值,超声心动图左室射血分数(LVEF)以及性别、年龄、民族等相关临床指标。按照纽约心功能分级(NYHA)将病例组分为轻症组(NYHAⅠ~Ⅱ)及重症组(NYHAⅢ~Ⅳ)。按照LEVF下降程度将病历组分为LEVF轻度下降组(LVEF 40%~50%)及中重度下降组LVEF<40%。分别比较心功能不全患者与正常人,NYHA分级严重程度不同的患者之间相较,LEVF下降程度不同的患者之间相较,PtfV1数值的差异。并分析PtfV1与传统评价心功能严重程度的指标LVEF之间的相关性。结果 1心功能不全患者与对照组相较,PtfV1数值明显下降(p<0.05);2NYHA分级重症心功能不全患者较轻症患者的PtfV1数值明显下降(p<0.05);3LVEF中重度降低患者与轻度降低的患者相较,Ptfv1数值明显下降(p<0.05);4PtfV1与LVEF呈显著正相关,相关系数r=0.77,p<0.01。结论 V1导联P波终末电势(PtfV1)可作为评价心功能不全患者病情严重程度的一项临床心电学指标。展开更多
基金supported by the National Natural Science Foundation of China (NSFC,grant Nos.12494571,11963001 and 12133003)supported by the Program of Bagui Scholars (LHJ)。
文摘In this paper,we determine the photosphere evolution of PTF11rka which is a type Ic supernova (SN) by fitting its spectral energy distributions at different epochs.We find that the photosphere of PTF11rka expanded at a constant velocity at early epochs,and the photosphere temperature increased slightly after reaching a minimum.These features are reminiscent of those of SN 2017dio.Based on the photosphere module that can describe the photosphere evolution of PTF11rka,we use the ^(56)Ni cascade decay model to fit its multiband light curves (LCs),finding that the model can well fit the photometric data.The derived ejecta mass and ^(56)Ni mass are respectively 8.76■ and 0.29-0.41■;the derived peak luminosity and the rise time of the theoretical bolometric LC of PTF11rka are ~8.24×10^(42)erg s^(-1) and ~35 days,respectively.Moreover,we find that the theoretical multiband LCs and the theoretical bolometric LC of PTF11rka do not show early-time excesses proposed in the literature.This indicates that additional energy sources (e.g.,the interaction between the ejecta and the circumstellar material)suggested to be responsible for the early-time excess can be neglected.
基金supported by National Natural Science Foundation of China(NSFC,grant Nos.11963001,12133003,11833003,11973020(C0035736),and U1938201)supported by the Guangxi Talent Program(“Highland of Innovation Talents”)。
文摘In this paper,we perform the detailed modeling for the light curves(LCs)of PTF 10iuv which is a calcium-rich(Ca-rich)supernova(SN)to constrain the physical properties of its ejecta and the energy sources,as well as the explosion mechanism.We find that the^(56)Ni model and the56Ni plus circumstellar interaction model fail to explain the LCs,while the four-element(^(56)Ni,^(48)Cr,^(52)Fe,and^(44)Ti)model can account for the LCs.The ejecta mass of PTF10iuv derived by the model(1.52_(-0.25)^(+0.34)M_(⊙))is consistent with that of the merger of a sub-Chandrasekhar mass white dwarf.The early-time LCs were mainly powered by^(56)Ni whose mass is~0.03 M_(⊙),while the contributions of^(48)Cr and^(52)Fe can be neglected.The derived^(44)Ti mass(~0.25 M_(⊙))is~1.8 times the upper limit of the derived^(44)Ti mass of Ca-rich SN 2005E.We suggest that subtracting the contributions of the host-galaxy,which are unknown,and including the flux from other long-lived elements(e.g.,^(57)Co,^(55)Fe,^(60)Co)can reduce the amount of^(44)Ti,and that this value can be regarded as an upper limit.
文摘目的探讨V1导联P波终末电势(P wave terminal force in lead V1,PtfV1)在心功能不全患者中的临床应用价值。方法 110例心功能不全患者及100例正常对照组纳入研究。测量、计算、记录所有入选者的体表心电图PtfV1数值,超声心动图左室射血分数(LVEF)以及性别、年龄、民族等相关临床指标。按照纽约心功能分级(NYHA)将病例组分为轻症组(NYHAⅠ~Ⅱ)及重症组(NYHAⅢ~Ⅳ)。按照LEVF下降程度将病历组分为LEVF轻度下降组(LVEF 40%~50%)及中重度下降组LVEF<40%。分别比较心功能不全患者与正常人,NYHA分级严重程度不同的患者之间相较,LEVF下降程度不同的患者之间相较,PtfV1数值的差异。并分析PtfV1与传统评价心功能严重程度的指标LVEF之间的相关性。结果 1心功能不全患者与对照组相较,PtfV1数值明显下降(p<0.05);2NYHA分级重症心功能不全患者较轻症患者的PtfV1数值明显下降(p<0.05);3LVEF中重度降低患者与轻度降低的患者相较,Ptfv1数值明显下降(p<0.05);4PtfV1与LVEF呈显著正相关,相关系数r=0.77,p<0.01。结论 V1导联P波终末电势(PtfV1)可作为评价心功能不全患者病情严重程度的一项临床心电学指标。
