The eclipsing LMC star OGLE 05155332-6925581: a clue for double periodic variables
We investigate the nature of OGLE05155332-6925581, one of the brightest members of the enigmatic group of double periodic variables (DPVs) recently found in the Magellanic Clouds. The modelling of archival orbital light curves (LCs), along with the analysis of the radial velocities (RVs) suggest tha...
Guardado en:
| Autores principales: | , , , , , , , |
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| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2008
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/93755 https://academic.oup.com/mnras/article/389/4/1605/1103880 https://ri.conicet.gov.ar/handle/11336/45717 |
| Aporte de: |
| id |
I19-R120-10915-93755 |
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| record_format |
dspace |
| institution |
Universidad Nacional de La Plata |
| institution_str |
I-19 |
| repository_str |
R-120 |
| collection |
SEDICI (UNLP) |
| language |
Inglés |
| topic |
Astronomía binaries: eclipsing stars: early-type stars: evolution stars: mass-loss stars: variables: other |
| spellingShingle |
Astronomía binaries: eclipsing stars: early-type stars: evolution stars: mass-loss stars: variables: other Mennickent, R. E. Kolaczkowski, Z. Michalska, G. Pietrzyński, G. Gallardo, R. Cidale, Lydia Sonia Granada, Anahí Gieren, W. The eclipsing LMC star OGLE 05155332-6925581: a clue for double periodic variables |
| topic_facet |
Astronomía binaries: eclipsing stars: early-type stars: evolution stars: mass-loss stars: variables: other |
| description |
We investigate the nature of OGLE05155332-6925581, one of the brightest members of the enigmatic group of double periodic variables (DPVs) recently found in the Magellanic Clouds. The modelling of archival orbital light curves (LCs), along with the analysis of the radial velocities (RVs) suggest that this object is a semidetached binary with the less massive star transferring matter to the more massive and less evolved star, in an Algol-like configuration. We find evidence for additional orbital variability and Hα emission, likely caused by an accretion disc around the primary star. As in the case of β Lyr the circumprimary disc seems to be more luminous than the primary, but we do not detect orbital period changes. We find that the LC follows a loop in the colour-magnitude diagram during the long cycle; the system is redder when brighter and the rising phase is bluer than during decline. Infrared excess is also present. The source of the long-term periodicity is not eclipsed, indicating its circumbinary origin. Strong asymmetries, discrete absorption components (DACs) and a γ shift are new and essential observational properties in the infrared HI lines. The DACs strength and RV follow a saw-teeth pattern during the orbital cycle. We suggest that the system experiences supercycles of mass outflow feeding a circumbinary disc. Mass exchange and mass loss could produce comparable but opposite effects in the orbital period on a long time-scale, resulting in a quasi-constancy of this parameter. |
| format |
Articulo Articulo |
| author |
Mennickent, R. E. Kolaczkowski, Z. Michalska, G. Pietrzyński, G. Gallardo, R. Cidale, Lydia Sonia Granada, Anahí Gieren, W. |
| author_facet |
Mennickent, R. E. Kolaczkowski, Z. Michalska, G. Pietrzyński, G. Gallardo, R. Cidale, Lydia Sonia Granada, Anahí Gieren, W. |
| author_sort |
Mennickent, R. E. |
| title |
The eclipsing LMC star OGLE 05155332-6925581: a clue for double periodic variables |
| title_short |
The eclipsing LMC star OGLE 05155332-6925581: a clue for double periodic variables |
| title_full |
The eclipsing LMC star OGLE 05155332-6925581: a clue for double periodic variables |
| title_fullStr |
The eclipsing LMC star OGLE 05155332-6925581: a clue for double periodic variables |
| title_full_unstemmed |
The eclipsing LMC star OGLE 05155332-6925581: a clue for double periodic variables |
| title_sort |
eclipsing lmc star ogle 05155332-6925581: a clue for double periodic variables |
| publishDate |
2008 |
| url |
http://sedici.unlp.edu.ar/handle/10915/93755 https://academic.oup.com/mnras/article/389/4/1605/1103880 https://ri.conicet.gov.ar/handle/11336/45717 |
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