Open Access

Table 2

Sample of ULLYSES targets. O-type stars in the N11 B star-forming region in the LMC.

# ID Cross ID Coordinates (J2000)(a) Mv E(B – V) SpC vr Binary
RA Dec (mag) (mag) (km s–1)(c) status
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
1 PGMW 3053 N11 18 04:56:41.05 –66:24:40.54 –5.8 0.15 O6.5 II(f)(c) 301 Single(†)
2 PGMW 3058 N11 60 04:56:42.15 –66:24:54.61 –5.0 0.19 O3 V((f*))(c) 314 Single(†)
3 PGMW 3061 N11 31 04:56:42.51 –66:25:18.22 –5.7 0.22 ON2 III(f*)(d) 322 Single(†)
4 PGMW 3100 N11 38 04:56:45.20 –66:25:10.78 –5.7 0.26 O5 III(f)(c) 318 SB1
5 PGMW 3120a 04:56:46.80 –66:24:46.86 –6.7 0.21 O5.5 V((f))(c) 300 Cluster(††)
6 PGMW 3168 N11 32 04:56:54.46 –66:24:15.87 –5.3 0.16 O7.5 III(f)(c) 305 Single(†)
7 PGMW 3204 N11 48 04:56:58.79(b) -66:24:40.71(b) –5.0 0.16 O6Vz((f))(c) 299 Single(†)
8 PGMW 3223 N11 13 04:57:00.88 –66:24:25.21 –6.2 0.19 O8 Vz(c) SB1

Notes. (1) Object #; (2) PGMW# identification (ID) from Parker et al. (1992); (3) N11 # ID from Evans et al. (2006); (4) right ascension (J2000); (5) declination (J2000); (6) absolute visual magnitude (this work); (7) reddening (this work); (8) spectral type classification; (9) radial velocity (Evans et al. 2006); (10) binarity status (this work). (a)Gaia Collaboration (2020); (b)Bonanos et al. (2009); (c)PAC priv. comm.; (d)Evans et al. (2006); (†)Here, single means without evidence of binarity. SB1 status was determined here based on GIRAFFE multi-epoch spectra (see text for details). (††)PGMW 3120a is one of three stars of around the same brightness clustering (with PGMW 3120b,c) in the source known as PGMW 3120 (see Fig. 2 and text for details).

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.