We study the influence of host galaxy morphology on LC parameters of the JLA data.
The α parameter decreases from elliptical/lenticular to late-type spiral galaxies.
In an old stellar population SNe Ia are fainter after stretch and colour corrections.
The host galaxy morphology affects the residual dispersion on the Hubble diagram.
SNe Ia in late-type spiral galaxies are more homogeneous in comparison with others.
© 2004-2018 中国地质图书馆版权所有 京ICP备05064691号 京公网安备11010802017129号 地址:北京市海淀区学院路29号 邮编:100083 电话:办公室:(+86 10)66554848;文献借阅、咨询服务、科技查新:66554700 |