Table 6.
Atmospheric parameters of hot UV-bright stars from refereed publications until 2019-03-01.
| Cluster | Star | Teff | log g |  |
Status | Ref. | V | Ref. | M |
|---|---|---|---|---|---|---|---|---|---|
| (K) | (cm s−2) | (mag) | (M⊙) | ||||||
| NGC 104 | BS | 11 000 | 2.5 | −1 | pAGB | (1) | 10.73 | (13) | 1.25 |
| NGC 1851 | UV5 | 16 000 | 2.5 | −1 | pAGB | (2) | 13.26 | (14) | 0.41 |
| NGC 5139 | ROA5701 | 25 000 | 3.3 | −1 | pAGB | (3) | 13.13 | (24) | 0.32 |
| NGC 5272 | vZ1128 | 36 600 | 3.95 | −0.84 | peAGB | (4) | 15.03 | (15) | 0.41 |
| NGC 5904 | ZNG1 | 44 300 | 4.3 | +0.52 | pAGB | (5) | 14.54 | (16) | 0.72 |
| NGC 5986 | ID6 | 8750 | 2.0 | −1.4 | pAGB | (12) | 12.65 | (22) | 1.21 |
| NGC 6205 | B29 | 21 400 | 3.10 | −0.89 | pAGB | (6) | 13.116 | (23) | 0.38 |
| NGC 6254 | ZNG1 | 27 000 | 3.6 | −1.33 | pAGB | (7) | 13.23 | (17) | 0.59 |
| NGC 6397 | ROB162 | 51 000 | 4.5 | −1.0 | pAGB | (8) | 13.1 | (9) | 0.50 |
| NGC 6656 | II-81 | 38 000 | 4.2 | pHB | (9) | 14.0 | (18) | 0.47 | |
| NGC 6712 | ZNG1 | 11 000 | 2.1 | −1.19 | pAGB | (7) | 13.33 | (19) | 0.35 |
| NGC 6752 | B852 | 39 000 | 5.2 | −2.0 | pHB | (10) | 15.91 | (20) | 0.52 |
| B4380 | 32 000 | 5.3 | −2.3 | pHB | (10) | 15.93 | (20) | 0.79 | |
| B1754 | 40 000 | 5.0 | −1.52 | pHB | (10) | 15.99 | (20) | 0.30 | |
| NGC 7078 | K648 | 39 000 | 3.9 | −1.10 | pAGB | (11) | 14.73 | (11) | 0.62 |
| K996 | 11 500 | 2.5 | pHB | (12) | 14.31 | (21) | 0.26 | ||
| ZNG1 | 28 000 | 3.7 | −1.22 | pAGB | (7) | 14.8 | (17) | 0.55 |
Notes. The masses were derived by us as described in Sect. 6.
References. (1) Dixon et al. (1995); (2) Dixon et al. (1994); (3) Thompson et al. (2007); (4) Chayer et al. (2015); (5) Dixon et al. (2004); (6) Dixon et al. (2019); (7) Mooney et al. (2004); (8) Heber & Kudritzki (1986); (9) Glaspey et al. (1985); (10) Moehler et al. (1997); (11) Rauch et al. (2002); (12) Jasniewicz et al. (2004). (13) Lloyd Evans (1974) (14) Walker (1992) (15) Buzzoni et al. (1992) (16) Piotto et al. (2002) (17) de Boer (1987) (18) Arp & Melbourne (1959) (19) Cudworth (1988) (20) Buonanno et al. (1986) (21) Buonanno et al. (1983) (22) Alves et al. (2001) (23) Sandquist et al. (2010) (24) Bellini et al. (2009).
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