Soft band X/K luminosity ratios in late-type galaxies and constraints on the population of supersoft X-ray sources

TL;DR

This study examines the X-ray to K-band luminosity ratios in late-type galaxies to understand the contribution of supersoft X-ray sources to type Ia supernovae, using Chandra data and HI maps.

Contribution

It provides new measurements of L_X/L_K ratios in late-type galaxies and constrains the role of supersoft X-ray sources as SN Ia progenitors.

Findings

L_X/L_K ratios range from 5.4 to 68 x 10^27 erg/s/L_K,sun.

Supersoft X-ray sources contribute at most 15% to SN Ia rate in most galaxies.

Interstellar absorption significantly affects X-ray luminosity measurements.

Abstract

We study X-ray to K-band luminosity ratios (L_X/L_K) of late-type galaxies in the 0.3-0.7 keV energy range. From the Chandra archive, we selected nine spiral and three irregular galaxies with point source detection sensitivity better than 5 x 10^36 erg/s in order to minimize the contribution of unresolved X-ray binaries. In late-type galaxies cold gas and dust may cause significant interstellar absorption, therefore we also demanded the existence of publicly available HI maps. The obtained L_X/L_K ratios vary between (5.4-68) x 10^27 erg/s/L_K,sun exceeding by factor of 2-20 the values obtained for gas-poor early-type galaxies. Based on these results we constrain the role of supersoft X-ray sources as progenitors of type Ia supernovae (SNe Ia). For majority of galaxies the upper limits range from ~3% to ~15% of the SN Ia frequency inferred from K-band luminosity, but for a few of them no meaningful constraints can be placed. On a more detailed level, we study individual structural components of spiral galaxies: bulge and disk, and, for grand design spiral galaxies, arm and interarm regions.