Unveiling the Dual Nature of V1180 Cas: UXor-like Dips and EXor-like Bursts across a Decade
Open Access
- 10 February 2026
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 998 (2) , 204
Abstract
We present a detailed analysis of the long-term photometric and spectroscopic evolution of V1180 Cas over a decade, aiming to identify the dominant mechanisms behind its variability. We combine multiband light curves from 1999 to 2025 with over 30 epochs of optical to near-infrared (NIR) spectroscopy (0.5–2.5 μ m), analyzing variability patterns, color behavior, and emission line diagnostics. We investigate the temporal evolution of accretion and outflow indicators and their correlation with photometric states. The light curve reveals a transition from sporadic early dimming events to a quasi-periodic pattern since 2018, with 11 major dips showing asymmetry and stochastic substructure. Color–magnitude diagrams show classic UXor-like blueing during deep minima, while NIR and mid-infrared color changes indicate thermal evolution of the disk. Spectroscopic analysis reveals persistent hydrogen, Ca II , He I , and forbidden line emission. Accretion diagnostics track photometric variability, and forbidden lines often intensify during dips, implying a physical link between extinction and outflows. Estimated accretion rates range from ∼10 −8 to 10 −7 M ⊙ yr −1 ; the outflow rate and density diagnostics are consistent with disk winds and shock-excited jets. V1180 Cas demonstrates dual-mode variability driven by both variable circumstellar extinction and episodic accretion events. The hybrid UXor/EXor behavior, combined with evolving disk signatures and persistent outflows, suggests a young stellar object undergoing coupled accretion–extinction–outflow evolution. Continued monitoring will be essential to fully resolve the physical processes shaping its variability.Keywords
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Funding Information
- Department of Atomic Energy, Government of India (RTI 4002)
- Thailand Science Research and Innovation (FFB680072/0269)
- Department of Science and Technology, Ministry of Science and Technology, India (DST/INSPIRE 1375 Fellowship/2019/IF190550)
- Department of Science and Technology, Ministry of Science and Technology, India (DST/INSPIRE 1411 Fellowship/2022/IF220587)
- UNAM ∣ Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México (IN105225)
This publication has 83 references indexed in Scilit:
- Quiescence of an outburst of a low-mass young stellar object: LDN1415-IRSJournal of Astrophysics and Astronomy, 2023
- Spectroscopy of nine eruptive young variables using TANSPECJournal of Astrophysics and Astronomy, 2023
- pyTANSPEC: A data reduction package for TANSPECJournal of Astrophysics and Astronomy, 2023
- The Unusual Photometric Variability of the PMS Star GM CepPublications of the Astronomical Society of Australia, 2015
- PyNeb: a new tool for analyzing emission linesAstronomy & Astrophysics, 2014
- Recent outburst of the young star V1180 CassiopeiaeAstronomy & Astrophysics, 2014
- X-shooter spectroscopy of young stellar objectsAstronomy & Astrophysics, 2013
- Astropy: A community Python package for astronomyAstronomy & Astrophysics, 2013
- The outburst and nature of two young eruptive stars in the North America/Pelican Nebula ComplexAstronomy & Astrophysics, 2011
- Circumstellar disks and the search for neighbouring planetary systemsNature, 1996