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| Query : 2007BAVSR..56...14H |
2007BAVSR..56...14H - BAV Rundbrief, 56, 14-15 (2007/March-0)
HUND F.
Abstract (from CDS):
Light curves of CCD observations of ET Mus and HO Aps are showing the old classifications are wrong. ET Mus is a short period eclipsing binary with a period of 0.229689 ±0.000003d, Eo=2453922.51 ±0.003. HO Aps is an RRc Type pulsating star with a period of 0.584 ±0.005d, Eo=2453926.503 ±0.005.
Abstract Copyright: ∼
Journal keyword(s):
Simbad objects: 2
| Number of rows : 2 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | V* ET Mus | RR* | 12 57 29.5378479072 | -74 53 53.287747872 | ~ | 9 | 0 | |||||
| 2 | V* HO Aps | RR* | 16 12 09.0158619960 | -76 52 13.442978244 | ~ | 9 | 0 |
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