VdBH 222: a starburst cluster in the inner Milky Way

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Table 3

Parameters obtained for the nine brightest stars of the cluster using CHORIZOS code.

Name

T_eff

R₅₄₉₅

E(4405−5495)

E(B − V)

A _V

m_V − A_V

442

0.31

37.6 ± 7.5

2.78 ± 0.05

2.55 ± 0.05

2.46 ± 0.05

7.04 ± 0.09

9.19 ± 0.07

516

1.93

41.8 ± 5.5

2.90 ± 0.05

2.60 ± 0.03

2.51 ± 0.03

7.48 ± 0.06

8.86 ± 0.04

520^a

10.00

33.3 ± 8.6

2.85 ± 0.06

2.72 ± 0.07

2.61 ± 0.07

7.68 ± 0.11

8.88 ± 0.11

589

1.12

36.5 ± 7.8

2.75 ± 0.05

2.82 ± 0.05

2.70 ± 0.05

7.68 ± 0.09

9.28 ± 0.08

601

2.72

38.3 ± 7.1

3.27 ± 0.06

2.56 ± 0.04

2.48 ± 0.04

8.31 ± 0.08

8.44 ± 0.06

627

1.46

24.3 ± 5.4

2.97 ± 0.07

2.60 ± 0.08

2.50 ± 0.08

7.66 ± 0.13

9.76 ± 0.13

637

3.15

33.6 ± 4.5

2.90 ± 0.05

2.69 ± 0.04

2.59 ± 0.04

7.75 ± 0.08

9.63 ± 0.07

697

0.12

35.4 ± 8.1

2.79 ± 0.05

2.60 ± 0.06

2.51 ± 0.05

7.19 ± 0.10

9.55 ± 0.09

705

4.79

37.8 ± 7.6

2.68 ± 0.05

2.87 ± 0.05

2.74 ± 0.05

7.60 ± 0.09

9.38 ± 0.08

Notes.

^(a)

Inspection of the IR images suggests that the star is blended with another object so its JHK_S magnitudes are suspect.

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