MUSE observations of the blue compact dwarf galaxy Haro 14 - Data analysis and first results on morphology and stellar populations

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Volume 654 (October 2021)

A&A, 654 (2021) A142

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Table 4.

Properties of the emission-line sources detected in Haro 14.

Reg	ΔX	ΔY	Area	FWHM	F(Hα)	F([OIII])	log(L_Hα)	log(L_[OIII])
	(arcsec)	(arcsec)	(arcsec²)	(arcsec)	(erg s⁻¹ cm⁻²)	(erg s⁻¹ cm⁻²)	(erg s⁻¹)	(erg s⁻¹)
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)
L01	−0.4	1.9	4.96	1.07	36.720	43.350	38.9	38.9
L02	3.0	−4.0	4.56	1.18	16.396	14.470	38.5	38.5
L03	−7.9	3.3	6.64	1.51	21.026	23.103	38.6	38.7
L04	−5.4	2.9	1.20	1.18	2.442	1.895	37.7	37.6
L05	0.0	8.3	1.52	1.31	2.700	1.797	37.7	37.6
L06	1.4	9.1	1.16	1.23	2.081	1.536	37.6	37.5
L07	2.7	−11.1	6.16	2.09	8.189	5.814	38.2	38.1
L08	−3.7	−2.1	6.56	1.45	4.444	4.510	38.0	38.0
L09	0.7	4.4	6.16	1.62	5.578	4.446	38.1	38.0
L10	3.5	2.0	4.48	1.25	1.850	1.143	37.6	37.4
L11	−12.5	6.8	2.28	1.05	1.091	0.331	37.3	36.8
L12	−11.2	3.4	1.32	1.16	0.597	0.347	37.1	36.8
L13	4.1	−1.4	6.68	2.09	1.772	0.436	37.6	36.9
L14	−14.3	7.2	1.80	1.31	0.845	0.151	37.2	36.5
L15	−2.3	12.5	3.28	2.05	1.513	0.568	37.5	37.1
L16	−2.6	10.6	1.16	1.23	0.317	0.172	36.8	36.5
L17	−14.2	12.5	6.64	1.45	1.359	0.267	37.4	36.7
L18	−1.5	−4.1	3.24	1.67	0.285	0.009	36.8	35.3
L19	−8.7	6.4	1.20	0.97	0.079	0.000	36.2	22.1
L20	−7.8	−6.2	6.04	1.38	0.284	0.078	36.8	36.2
L21	−9.3	7.9	3.04	0.97	0.116	0.016	36.4	35.5
L22	−7.4	10.9	6.20	2.07	0.468	0.078	37.0	36.2
L23	5.4	4.0	1.28	0.83	0.083	0.031	36.2	35.8
L24	−2.3	−10.1	6.08	1.89	0.237	0.115	36.7	36.4
L25	11.1	−0.6	5.44	1.97	0.181	0.417	36.6	36.9
L26	−18.0	3.9	6.40	1.70	0.138	0.269	36.4	36.7
L27	−13.5	−4.0	2.64	1.09	0.036	0.059	35.9	36.1
L28	13.1	0.2	2.12	1.51	0.078	0.136	36.2	36.4
L29	−16.9	−2.3	5.40	1.62	0.034	0.025	35.8	35.7
L30	−9.0	−10.1	6.32	1.97	0.073	0.014	36.2	35.5
L31	−24.7	5.0	6.72	1.00	0.035	0.008	35.9	35.2
L32	−26.4	1.7	6.08	1.05	0.048	0.015	36.0	35.5
L33	−19.8	7.1	4.96	1.80	0.021	0.003	35.6	34.8
L34	8.4	−15.4	1.44	1.36	0.004	0.002	34.9	34.6
L35	−20.5	0.0	6.12	2.22	0.013	0.010	35.4	35.3
L36	−21.0	11.0	1.72	1.49	0.006	0.004	35.0	34.9
L37	1.7	−23.9	6.48	2.37	0.025	0.003	35.7	34.8
L38	23.6	−0.5	6.72	2.13	0.024	0.050	35.7	36.0
L39	12.1	−28.4	6.32	2.37	0.008	0.005	35.2	35.0
L40	−7.2	29.2	6.80	1.59	0.002	0.004	34.6	35.0
L41	−6.3	1.0	2.80	1.36	0.167	0.651	36.5	37.1
L42	−6.5	−0.5	1.28	1.29	1.550	0.769	37.5	37.2
L43	3.8	−8.5	4.16	1.62	2.272	2.157	37.7	37.6
L44	−9.1	−5.4	6.08	1.88	0.237	0.578	36.7	37.1
L45	−15.5	11.7	1.04	1.05	0.060	0.050	36.1	36.0
L46	−5.2	−6.8	4.24	0.80	0.003	0.000	34.8	28.0
L47	−7.2	−8.1	2.20	1.09	0.081	0.047	36.2	36.0
L48	−0.1	−13.8	1.24	1.20	0.008	0.029	35.2	35.8
L49	−14.3	0.0	2.52	1.05	0.076	0.023	36.2	35.7
L50	−12.6	−1.7	1.28	0.70	0.001	0.006	34.3	35.1
L51	−17.2	15.0	6.72	1.33	0.041	0.055	35.9	36.0
L52	5.4	−18.3	6.20	1.70	0.015	0.039	35.5	35.9
L53	14.1	−12.0	6.08	1.64	0.007	0.039	35.2	35.9
L54	17.3	−9.7	6.08	1.64	0.011	0.014	35.3	35.5
L55	−12.9	−15.4	6.44	1.78	0.012	0.010	35.4	35.3

Notes. Columns (2) and (3) display the offsets in arcsec from the position of the continuum peak. Fluxes are in units of 10⁻¹⁵ erg s⁻¹ cm⁻². Fluxes and luminosities (Cols. 6–9) are corrected from Galactic extinction using the reddening coefficients from Schlafly & Finkbeiner (2011).

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