An Unusual Eclipse of a Pre-Main Sequence Star in IC 348
arXiv:astro-ph/0308484 · doi:10.1086/379275
Abstract
A solar-like pre-main sequence star (TJ 108 = H 187 = LRLL 35 = HMW 15) in the extremely young cluster IC 348 has been found, which apparently experienced an eclipse lasting ~3.5 years, much longer than has ever been detected for any normal eclipsing binary. The light curve is flat-bottomed and rather symmetric, with a depth of 0.66 mag in Cousins I. During eclipse, the system reddened by \~0.17 mag in R-I. We argue that the eclipsing body is not a star because of the small probability of detecting an eclipse in what would be a very widely separated binary. Instead, it appears that the eclipse was caused by a circumstellar or circumbinary cloud or disk feature which occulted the star, or one of its components, if it is a binary system. We emphasize the importance of more detailed study of this object, which appears to be a new member of a small class of pre-main sequence stars whose variability can be firmly linked to occultation by circumstellar (or circumbinary) matter.
13 pages, 2 figures
References in corpus (4)
- A Census of the Young Cluster IC 348
- Eclipses by a Circumstellar Dust Feature in the Pre-Main Sequence Star KH15D
- Fine Structure in the Circumstellar Environment of a Young, Solar-like Star: the Unique Eclipses of KH 15D
- A Variability Study of Pre-Main Sequence Stars in the Extremely Young Cluster IC 348
Cited by in corpus (8)
- CSI 2264: Simultaneous optical and infrared light curves of young disk-bearing stars in NGC 2264 with CoRoT and Spitzer-- evidence for multiple origins of variability
- A Multi-Year Photometric Study of IC 348
- The unusual pre-main-sequence star V718 Per (HMW 15)
- Long-Term Photometry of IC 348 with the YETI Network
- Modulation of Circumstellar Extinction in a Young Binary System with a Low-Mass Companion in a Noncoplanar Orbit
- Inhomogeneous dust eclipses in young stars. The case of CQ Tauri
- The Recurrent Eclipse of an Unusual Pre--Main-Sequence Star in IC 348
- Interpretation of a Variable Reflection Nebula Associated with HBC 340 and HBC 341 in NGC 1333