Abstract
The Advanced CCD Imaging Spectrometer (ACIS-S) camera on board the Chandra X-ray Observatory has been used to discover a hot bubble in the planetary nebula (PN) IC 4593, the most distant PN detected by Chandra so far. The data are used to study the distribution of the X-ray-emitting gas in IC 4593 and to estimate its physical properties. The hot bubble has a radius of ~2 arcsec and is found to be confined inside the optically bright innermost cavity of IC 4593. The X-ray emission is mostly consistent with that of an optically thin plasma with temperature kT ~0.15 keV (or TX ~1.7 × 106 K), electron density ne ~15 cm-3, and intrinsic X-ray luminosity in the 0.3-1.5 keV energy range LX = 3.4 × 1030 erg s-1. A careful analysis of the distribution of hard (E >0.8 keV) photons in IC 4593 suggests the presence of X-ray emission from a point source likely associated with its central star (CSPN). If this was the case, its estimated X-ray luminosity would be LX, CSPN = 7 × 1029 erg s-1, fulfilling the log(LX, CSPN/Lbol)~-7 relation for self-shocking winds in hot stars. The X-ray detection of the CSPN helps explain the presence of high-ionization species detected in the ultraviolet spectra as predicted by stellar atmosphere models.
Original language | English (US) |
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Pages (from-to) | 3784-3789 |
Number of pages | 6 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 494 |
Issue number | 3 |
DOIs | |
State | Published - 2020 |
Externally published | Yes |
Keywords
- Planetary nebulae: IC 4593 -X-rays: general
- Planetary nebulae: general
- Stars: low-mass
- Stars: winds, outflows
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science