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Table 3

Intergalactic HII regions candidates in the environment of NGC 2865.

ID α δ λ FWHM V sys a FluxHα
(J2000) (J2000) Å Å km s-1 erg s-1 cm-2

NGC 2865b 09h 23m 30 2 − 23° 09 41.̋0 2627
IG_04_P0 09h23m36 − 23° 09 15.̋8 6621 7.2 2666 2.6e-16
IG_04_P3 09h23m36 − 23° 09 15.̋8 6624 5.9 2811 1.9e-16
IG_04_P4 09h23m36 − 23° 09 15.̋8 6620 7.2 2628 3.2e-16
IG_87_P0 09h23m439 − 23° 13 08.̋9 6630 7.3 3070 3.6e-16
IG_17_P1 09h23m309 − 23° 11 05.̋6 6623 7.9 2789 1.1e-16
IG_51_P3 09h23m366 − 23° 11 38.̋2 6619 6.3 2606 1.5e-16
IG_85_P6 09h23m411 − 23° 12 20.̋8 6617 5.1 2507 1.0e-16
IG_52_P7 09h23m402 − 23° 12 12.̋7 6618 5.8 2568 1.4e-16
IG_23_P8 09h23m305 − 23° 11 36.̋4 6624 5.7 2828 9.0e-17

Notes.

(a)

Systemic velocities deduced from our Hα line analysis. Heliocentric velocities given by the task rvidline from iraf. The errors for the velocities were estimated using Monte Carlo simulation for 100 runs, and they are about 40 km s-1 for all the spectra.

(b)

For the main galaxy, NGC 2865, the value for its radial velocity was taken from Smith et al. (2000).

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