The first spectra for the RX J0440.9+4431 from 2m Terskol telescope
Andrew Simon (1), A. V. Bondar (2), V. M. Reshetnyk (1) ((1) National, Taras Shevchenko University of Kyiv, Glushkova ave., Kyiv, Ukraine, (2), International Center for Astronomical, Medical, Ecological Research,, Terskol Observatory)

TL;DR
This paper reports the first spectral observations of the Be/X-ray binary RX J0440.9+4431 using the 2m Terskol telescope, revealing V/R variability and disc change timescales.
Contribution
First spectral analysis of RX J0440.9+4431 from the Terskol observatory, providing new insights into its emission line profiles and disc variability.
Findings
V/R variability in H-alpha line profile
Estimated disc change timescale of about 14 years
Comparison with previous spectral data
Abstract
We present the first results on the spectra of Be/X-ray binary RX J0440.9+4431 obtained with the 2m Ritchey-Cretein-Coude telescope with Cassegrain Multi Mode Spectrograph (CMMS) (with R = 14000) at Terskol observatory. The H-alpha line profile indicates that the new episode of the V/R variability is occuring in the system. The profiles of the H-alpha, H-beta and HeI 7065.71, 6678.15, 5875.97 lines were analyzed and equivalent width were determined. We compared our H-alpha line profile parameters with the previous results from the literature and estimated characteristic time scale for disc changes as about 14 years.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAstrophysical Phenomena and Observations · Pulsars and Gravitational Waves Research · Adaptive optics and wavefront sensing
