On the light-curves of disk and bulge novae

Fuente: arXiv
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Hauptverfasser: Cohen, Asaf, Guetta, Dafne, Hillman, Yael, Della Valle, Massimo, Izzo, Luca, Perdelwitz, Volker, Livio, Mario
Format: Preprint
Veröffentlicht: 2025
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author Cohen, Asaf
Guetta, Dafne
Hillman, Yael
Della Valle, Massimo
Izzo, Luca
Perdelwitz, Volker
Livio, Mario
author_facet Cohen, Asaf
Guetta, Dafne
Hillman, Yael
Della Valle, Massimo
Izzo, Luca
Perdelwitz, Volker
Livio, Mario
contents We examine the light curves of a sample of novae, classifying them into single-peaked and multiple-peaked morphologies. Using accurate distances from Gaia, we determine the spatial distribution of these novae by computing their heights, $Z$, above the Galactic plane. We show that novae exhibiting a single peak in their light curves tend to concentrate near the Galactic plane, while those displaying multiple peaks are more homogeneously distributed, reaching heights up to 1000 pc above the plane. A KS test rejects the null hypothesis that the two distributions originate from the same population at a significance level corresponding to $4.2σ$.
format Preprint
id arxiv_https___arxiv_org_abs_2502_08198
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle On the light-curves of disk and bulge novae
Cohen, Asaf
Guetta, Dafne
Hillman, Yael
Della Valle, Massimo
Izzo, Luca
Perdelwitz, Volker
Livio, Mario
Astrophysics of Galaxies
Solar and Stellar Astrophysics
We examine the light curves of a sample of novae, classifying them into single-peaked and multiple-peaked morphologies. Using accurate distances from Gaia, we determine the spatial distribution of these novae by computing their heights, $Z$, above the Galactic plane. We show that novae exhibiting a single peak in their light curves tend to concentrate near the Galactic plane, while those displaying multiple peaks are more homogeneously distributed, reaching heights up to 1000 pc above the plane. A KS test rejects the null hypothesis that the two distributions originate from the same population at a significance level corresponding to $4.2σ$.
title On the light-curves of disk and bulge novae
topic Astrophysics of Galaxies
Solar and Stellar Astrophysics
url https://arxiv.org/abs/2502.08198