Tidal interaction vs. ram pressure stripping effects as seen in X-rays - Hot gas in group and cluster galaxies

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Table 1

Basic astronomical properties of studied galaxies.

NGC	Morph.	Optical position^a	Incl.^a	Pos.	Proj. dist. to	Radial	log(L_B/L_⊙)^d
	type^a	α₂₀₀₀ δ₂₀₀₀		ang.^a	system centre^b	velocity^c
			[°]	[°]	[°]/[Mpc]	[km s^-1]

2276	SABc	7^h27^m143+85°45′16′′	40	110	0.1	240	10.67
4254	Sc	12^h18^m496+14°24′59′′	32	60	3.56/1.07	1130	10.53
4569	SABa	12^h36^m501+13°09′46′′	66	23	1.66/0.5	1530	10.70

Notes.

^(a)

Taken from HYPERLEDA database – http://leda.univ-lyon1.fr – see Paturel et al. (1983).

^(b)

For NGC 2276 a projected distance to the most massive galaxy NGC 2300 is provided.

^(c)

Relative to the IGM/ICM estimated using the redshift based velocities in the HYPERLEDA database.

^(d)

Intrinsic blue luminosities in solar luminosities – Tully 1988.

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