A global view of shocked plasma in the supernova remnant Puppis A provided by SRG/eROSITA

The Early Data Release of eROSITA and Mikhail Pavlinsky ART-XC on the SRG mission

Open Access

Table 2

Best-fit parameters for single (BB) and double (2BB) blackbody fits to the spectrum of the CCO.

	This work		Hui & Becker (2006)
	BB	2BB	BB	2BB
N_h (10²¹ cm⁻²)
kT₁ (keV)
R₁ (km)^(a)
kT₂ (keV)	…		…
R₂ (km)^(a)	…		…
F_a (10⁻¹² erg s⁻¹ cm⁻²)^(b)			4.42	4.88
F_u(10⁻¹²ergs⁻¹cm⁻²)^(c)			6.05	8.94

Notes. Errors were estimated using the built-in Xspec command. ^(a)Size of the circular emitting region converted assuming a distance of 1.3 kpc. ^(b)Observed (i.e., absorbed) flux of the source in the 0.5–10keV range.^(c)Absorption-corrected flux of the source in the 0.5–10keV range.

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