Deep Chandra observations of NGC 7457, the X-ray point source populations of a low-mass early-type galaxy
Abstract
We present the X-ray point source population of NGC 7457 based on 124 ks of Chandra observations. Previous deep Chandra observations of low-mass X-ray binaries (LMXBs) in early-type galaxies have typically targeted the large populations of massive galaxies. NGC 7457 is a nearby, early-type galaxy with a stellar luminosity of 1.7× 10^{10}{L_{K{⊙}}}, allowing us to investigate the populations in a relatively low-mass galaxy. We classify the detected X-ray sources into field LMXBs, globular cluster LMXBs and background active galactic nuclei based on identifying optical counterparts in new HST/ACS images. We detect 10 field LMXBs within the rext ellipse of NGC 7457 (with semimajor axis ∼9.1 kpc, ellipticity = 0.55). The corresponding number of LMXBs with X-ray luminosities (Lx)>2× 10^{37}{erg s^{-1}} per stellar luminosity is consistent with that observed in more massive galaxies, ∼7 per 10^{10} L_{K{⊙}}. We detect a small globular cluster population in these HST data and show that its colour distribution is likely bimodal and that its specific frequency is similar to that of other early-type galaxies. However, no X-ray emission is detected from any of these clusters. Using published data for other galaxies, we show that this non-detection is consistent with the small stellar mass of these clusters. We estimate that 0.11 (and 0.03) LMXBs are expected per 106M_{{⊙}} in metal-rich (and metal-poor) globular clusters. This corresponds to 1100 (and 330) LMXBs per 10^{10} L_{K{⊙}}, highlighting the enhanced formation efficiency of LMXBs in globular clusters. A nuclear X-ray source is detected, with Lx varying from 2.8 × 1038 to 6.8 × 1038 erg s-1. Combining this Lx with a published dynamical mass estimate for the central supermassive black hole in NGC 7457, we find that Lx/L_{Edd} varies from 0.5 × 10-6 to 1.3 × 10-6.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- April 2017
- DOI:
- 10.1093/mnras/stw3375
- arXiv:
- arXiv:1701.00482
- Bibcode:
- 2017MNRAS.466.4021P
- Keywords:
-
- galaxies: individual: NGC 7457;
- galaxies: star clusters: general;
- X-rays: binaries;
- X-rays: galaxies;
- Astrophysics - High Energy Astrophysical Phenomena;
- Astrophysics - Astrophysics of Galaxies
- E-Print:
- 9 pages, 7 figures, 1 table, accepted for publication in MNRAS