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Name
  MACHO 80.6708.4936  
AAVSO UID
000-BPW-064 (No observations)  
Constellation
Dorado Sequence
J2000.0
05 21 54.94 -69 21 50.4  (80.47892 -69.36400) Search nearby
B1950.0 05 22 16.43 -69 24 35.4
Galactic coord. 280.038 -33.104
Other names

(Internal only)
2MASS J05215492-6921500 EROS2-BC J052154-692150 EROS2-star lm001-0n-25687
GSC2.3 S1HP098700 Gaia DR3 4658083077041868544 MACHO J052154.8-692150
OGLE LMC-CEP-1718 OGLE LMC-ECL-32252 OGLE LMC-SC6 330185
OGLE LMC100.2 55731 OGLE LMC503.10.115453 OGLE-LMC-CEP-1718
TIC 179587639 UCAC4 104-011697 USNO-A2.0 0150-02970183
USNO-B1.0 0206-0095651 [AAA95] J052154.8-692150  
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Variability type
DCEPS+DCEPS+EA
Spectral type --
Mag. range
14.38 - 14.70 Ic
Discoverer C. Alcock et al. (MACHO)
Epoch
01 Apr 2004 (HJD 2453097.3722) Ephemeris
Outburst --
Period 2.4809333 d
Rise/eclipse dur. --
Remarks
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1 Otero, Sebastian Alberto Binary system with two cepheids. Elements for the brightest one given in the table. Combined range given. COmbined cepheid amplitude 0.25 Ic. Fainter cepheid elements are 2453044.8611 + 1.963667 d. x E. (2024arXiv240312390P). Eclipsing binary with elements 2455050.5 + 412.807 d. (ampl. 0.08 Ic) (2014ApJ...786...80G).
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References
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1 Pilecki, B.; Thompson, I. B.; Espinoza-Arancibia, F.; et al., 2024,
Cepheids with giant companions. II. Spectroscopic confirmation of nine new
double-lined binary systems composed of two Cepheids
2024arXiv240312390P
2 Gieren, W.; Pilecki, B.; Pietrzyński, G.; et al., 2014, The Araucaria
Project. OGLE-LMC-CEP-1718: An Exotic Eclipsing Binary System Composed of
Two Classical Overtone Cepheids in a 413 Day Orbit
2014ApJ...786...80G
3 Soszyński, I.; et al., 2008, The Optical Gravitational Lensing
Experiment. The OGLE-III Catalog of Variable Stars. I. Classical Cepheids
in the Large Magellanic Cloud
2008AcA....58..163S
4 Alcock, C.; et al., 1995, The MACHO Project LMC Variable Star
Inventory.I.Beat Cepheids-Conclusive Evidence for the Excitation of the
Second Overtone in Classical Cepheids
1995AJ....109.1653A
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Supporting Documents
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Revision History
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1 Otero, Sebastian Alberto 2024-04-01 23:57 UTC Type and elements from 2024arXiv240312390P. Range from OGLE data.