Normal or transitional? The evolution and properties of two type Ia supernovae in the Virgo cluster

TL;DR

This study analyzes two Type Ia supernovae in the Virgo cluster, revealing that intrinsic color differences can distinguish normal from transitional SNe Ia, which is crucial for improving their use in cosmology.

Contribution

It provides detailed photometric and spectroscopic data on two SNe Ia, demonstrating the importance of spectroscopic analysis for accurate classification and understanding of color diversity.

Findings

SN 2020nlb is a normal SN Ia with intrinsically red color due to lower temperature.

SN 2020ue exhibits properties of transitional SNe Ia but spectroscopically aligns with normal SNe Ia.

Spectroscopic indicators are essential for identifying intrinsic color variations in SNe Ia.

Abstract

Type Ia supernovae (SNe Ia) are among the most precise cosmological distance indicators used to study the expansion history of the Universe. The vast increase of SN Ia data due to large-scale astrophysical surveys has led to the discovery of a wide variety of SN Ia sub-classes, such as transitional and fast-declining SNe Ia. However, their distinct photometric and spectroscopic properties differentiate them from the population of normal SNe Ia such that their use as cosmological tools remains challenged. Here, we present a high-cadenced photometric and spectroscopic dataset of two SNe Ia, SNe 2020ue and 2020nlb, which were discovered in the nearby Virgo cluster of galaxies. Our study shows that SN 2020nlb is a normal SN Ia whose unusually red color is intrinsic, arising from a lower photospheric temperature rather than interstellar reddening, providing clear evidence that color diversity among normal SNe Ia can have a physical origin. In contrast, SN 2020ue has photometric properties, such as color evolution and light-curve decay rate, similar to those of transitional SNe, spectroscopically it is more aligned with normal SNe Ia. This is evident from spectroscopic indicators such as the pseudo-equivalent width of \ion{Si}{II} lines. Thus, such SNe Ia that are photometrically at the edge of the standard normal SNe Ia range may be missed in cosmological SNe Ia samples. Our results highlight that spectroscopic analysis of SNe Ia around peak brightness is crucial for identifying intrinsic color variations and constructing a more complete and physically homogeneous SN Ia sample for precision cosmology.