Exploring the archives: A search for novae in UVIT snapshots of M31
arXiv:2406.10006 · doi:10.3847/1538-4357/ad596b
Abstract
Extensive multi-wavelength studies of novae have been carried out in our galaxy and in M31 for decades. However, UV studies of extragalactic novae are limited, especially those in quiescence. For the first time, we present a UV catalog of novae in M31 using the archival AstroSat UVIT imaging data. We used two image subtraction techniques to retrieve objects located deep into the M31 central region. We have found 42 novae in total in the UVIT images, 15 of which have been detected in multiple filters in FUV and NUV. The novae detected at quiescence show signatures of accretion disk from their UV spectral energy distributions, whereas those in the outburst phase show signatures of pseudo-photosphere. A few novae were also detected in multiple epochs. Some show a near-constant FUV magnitude at quiescence, while others caught near the outburst reveal pre-eruption dips in their light curves. We conclude with a discussion on the significance of UV surveys in illuminating theoretical predictions for novae systems, including detecting the elusive early UV flash.
16 pages, 4 figures, 4 tables. Accepted for publication in ApJ
References in corpus (15)
- Array Programming with NumPy
- The Zwicky Transient Facility: System Overview, Performance, and First Results
- A Universal Decline Law of Classical Novae
- X-ray monitoring of optical novae in M31 from July 2004 to February 2005
- A UV and optical study of 18 old novae with Gaia DR2 distances: mass accretion rates, physical parameters, and MMRD
- The B & V Light Curves for Recurrent Nova T CrB From 1842--2022, the Unique Pre- and Post-Eruption High-States, the Complex Period Changes, and the Upcoming Eruption in 2025.51.3
- A SITELLE view of M31's central region - I: Calibrations and radial velocity catalogue of nearly 800 emission-line point-like sources
- In-orbit Performance of UVIT on ASTROSAT
- Physics of nova outbursts: A theoretical model of classical nova outbursts with self-consistent wind mass loss
- Multiwavelength observations of nova SMCN 2016-10a --- one of the brightest novae ever observed
- On the progenitors of Local Group Novae - I. The M31 Catalog
- UVIT observations of the Small Magellanic Cloud: Point source catalogue
- The January 2016 eruption of recurrent nova LMC 1968
- The Rate and Spatial Distribution of Novae in M31 as Determined by a Twenty-Year Survey
- Mixing fraction in classical novae