Table 6
Spectral types and photometry for stars in the region not covered by our photometry.
| Star | Spectral type | V | B − V | U − B | (B − V)0 | (U − B)0 | E(B − V) | E(U − B) | V 0 |
|
|
|||||||||
| GSC 05124-02627 | B3 III | 11.82 | 0.95 | 0.17 | −0.20 | −0.73 | 1.15 | 0.90 | 8.26 |
| GSC 05124-02567 | B9 IV | 12.04 | 0.76 | 0.50 | −0.07 | −0.19 | 0.83 | 0.69 | 9.47 |
| GSC 05124-02605 | B6 III-IVp Si | 12.66 | 0.85 | 0.25 | − | − | − | − | − |
| 2MASS J18363487-06372271 | B0.5 V | − | − | − | − | − | − | − | − |
Notes. The three GSC stars were observed with grism #16. UBV photometry is from Roslund (1963). The intrinsic colours from Fitzgerald (1970) are used to derive excesses and dereddened magnitudes. This is not attempted for the chemically peculiar star.
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.