86 GHz SiO maser survey of late-type stars in the Inner Galaxy - IV. SiO emission and infrared data for sources in the Scutum and Sagittarius-Carina arms, 20° <  l <  50°

M. Messineo; H.J. Habing; L. O. Sjouwerman; A. Omont; K. M. Menten

doi:10.1051/0004-6361/201730717

Home

All issues

Volume 619 (November 2018)

A&A, 619 (2018) A35

Full HTML

Free Access

Table C.1.

Luminosities of bright targets and of targets with broad maser lines.

ID	Long	A_K(field)	A_K(tot)	M_bol(kin)	M_bol(14.5)	V_lsr	FWHM	Comments	References
	(°)	(mag)	(mag)	(mag)	(mag)	(km s⁻¹)	(km s⁻¹)
436	29.85	0.12	..0	..	−8.4	..	..	M3I	(1)
444	29.67	1.16	0.88	..	−7.9	..	..	M2I	(2)
483	29.26	1.32	1.40	−5.6	−7.1	66.9	4.3	RSG^a	(3)
535	24.63	1.29	1.76	..	−5.0	..	..	RSG^a	(4)
31	−0.44	1.80	1.72	..	−7.3	−24.4	9.6	M_bol(14.5) < −7.2, long < 5°
75	0.77	1.36	1.20	..	−8.0	−38.1	3.3	M_bol(14.5) < −7.2, long < 5°
92	0.11	1.66	1.41	..	−8.2	119.4	2.9	M_bol(14.5 ) < −7.2, long < 5°, sRSG^b	(5)
116	2.49	1.75	1.40	..	−7.6	19.5	4.2	M_bol(14.5) < −7.2, long < 5°
128	2.70	1.51	1.60	..	−7.9	−16.4	4.5	M_bol(14.5) < −7.2, long < 5°
294	−1.00	2.23	2.37	..	−7.8	..	..	M_bol(14.5) < −7.2, long < 5°, sRSG^b	(5)
310	−0.55	2.79	2.42	..	−7.4	..	..	M_bol(14.5) < −7.2, long < 5°
244	20.40	0.96	0.99	−6.2	−7.1	89.1	3.3	M_bol(kin) < − 6.0, long > 20°
449	21.70	1.05	0.91	−6.3	−7.6	73.6	8.2	M_bol(kin) < − 6.0, long > 20°
456	22.46	1.61	1.36	−6.6	−7.3	111.1	3.5	M_bol(kin) < − 6.0, long > 20°
460	24.43	1.20	0.98	−6.2	−8.1	49.0	13.2	M_bol(kin) < − 6.0, long > 20°
473	26.59	0.72	0.65	−6.1	−7.0	96.8	6.0	M_bol(kin) < − 6.0, long > 20°
474	27.05	0.82	0.50	−6.4	−7.9	66.9	11.8	M_bol(kin) < − 6.0, long > 20°
484	30.94	0.56	0.35	−6.3	−7.7	69.2	7.3	M_bol(kin) < − 6.0, long > 20°
495	33.30	0.95	0.59	−6.1	−7.1	84.5	3.8	M_bol(kin) < − 6.0, long > 20°
15	−1.38	0.99	0.89	−6.9	−7.2	38.7	7.3	M_bol(kin) < − 6.0, long < 20°, FG^c
23	−1.29	1.22	1.07	−6.8	−7.0	56.5	2.8	M_bol(kin) < − 6.0, long < 20°, FG^c
113	1.98	1.31	1.13	−6.7	−7.1	31.7	13.9	M_bol(kin) < − 6.0, long < 20°, FG^c
129	3.82	0.47	0.36	−7.1	−7.7	38.0	13.9	M_bol(kin) < − 6.0, long < 20°, FG^c
130	4.49	0.68	0.52	−6.4	−6.9	52.8	3.2	M_bol(kin) < − 6.0, long < 20°, FG^c
160	6.96	0.82	0.82	−6.2	−7.3	39.9	7.8	M_bol(kin) < − 6.0, long < 20°, FG^c
71	0.32	1.84	2.12	..	−5.3	92.5	9.0	Remaining FWHM > 9
87	1.24	1.21	1.24	..	−7.2	−15.3	9.2	Remaining FWHM > 9
117	2.01	1.85	3.25	..	−5.6	22.2	16.3	Remaining FWHM > 9
135	3.81	1.20	1.46	..	−5.6	207.1	11.9	Remaining FWHM > 9
173	8.66	1.61	1.20	..	−7.5	−1.1	11.5	Remaining FWHM > 9
190	10.99	1.04	1.10	..	−6.4	58.1	9.1	Remaining FWHM > 9
203	14.31	0.91	3.14	..	−4.0	81.1	12.7	Remaining FWHM > 9
223	17.80	1.02	1.87	..	−5.2	143.9	13.4	Remaining FWHM > 9
232	17.92	1.10	1.45	..	−5.4	94.3	9.8	Remaining FWHM > 9
452	21.71	1.11	1.54	−5.7	−6.6	97.1	13.3	Remaining FWHM > 9
457	22.25	1.51	1.28	−4.3	−7.5	19.8	9.1	Remaining FWHM > 9
459	24.13	1.05	1.66	−5.5	−5.6	139.5	10.4	Remaining FWHM > 9
469	25.97	0.86	1.70	−4.3	−4.9	113.4	12.7	Remaining FWHM > 9
481	29.12	0.73	0.31	−3.2	−7.8	10.2	11.7	Remaining FWHM > 9
486	31.67	1.75	5.20	−4.2	−5.2	91.0	10.6	Remaining FWHM > 9
489	31.50	1.43	2.68	−4.7	−5.4	98.0	9.8	Remaining FWHM > 9
490	31.36	1.55	2.27	−4.0	−5.5	69.8	12.4	Remaining FWHM > 9
491	33.42	1.11	1.09	−4.2	−7.0	31.5	14.6	Remaining FWHM > 9
493	34.00	1.04	1.38	−5.0	−6.1	78.9	11.1	Remaining FWHM > 9
502	35.06	2.02	2.02	−5.4	−7.5	45.8	9.1	Remaining FWHM > 9
511	35.25	1.47	2.49	−0.9	−6.2	7.3	9.2	Remaining FWHM > 9
526	44.24	0.94	1.39	−3.2	−5.7	34.0	9.7	Remaining FWHM > 9
530	47.95	0.71	1.88	−4.0	−4.8	58.0	10.4	Remaining FWHM > 9
432	28.97	0.97	1.17	−5.4	−6.2	103.1	19.9	Remaining FWHM > 9

Notes. Identification numbers (ID) are followed by longitudes (Long), median extinction of surrounding stars A_K(field), total extinction of the targets A_K(tot) (Messineo et al. 2005), M_bol values obtained by adopting the near kinematic distances, M_bol(kin), M_bol values obtained by adopting a distance modulus of 14.5 mag, radial velocities, V_lsr, and the maser line FWHMs. References. 1 = Jura & Kleinmann (1990) ; 2 = Messineo et al. (2016); 3 = Clark et al. (2009); 4 = Negueruela et al. (2010); 5 = this work.

^(a)

RSG = Star photometrically reported as a probable RSG in previous studies.

^(b)

sRSG = Stars confirmed as RSGs in this work with the spectral indexes of Messineo et al. (2017).

^(c)

FG = Stars classified as likely foreground by Messineo et al. (2005), their A_{K_s} values are smaller than the average A_{K_s} of surrounding stars.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.