2021/11/03 by Erik Wischnewski, Wischnewski, Erik
Engineering · Physics and Astronomy · #Astronomical Observations and Instrumentation #Astrophysical Phenomena and Observations #FOS: Physical sciences #Gamma-ray bursts and supernovae #Solar and Stellar Astrophysics (astro-ph.SR)
paper · pdf · doi:10.48550/arxiv.2111.02463
openalex publication_date 2021/11/03 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
CONTEXT: The Nova V1405 Cas, which erupted on 18 March 2021, showed a pre-maximum phase of almost two months. After the main maximum, during several month the nova only weakened slightly and showed clear fluctuations in brightness. AIMS: The aim of this work is to investigate the relationship between brightness and half-width (FWHM) and equivalent width (EW) of the H-alpha emission line, and from this to infer possible causes for the abnormal behavior of the Nova. METHODS: Magnitudes and spectra from online databases were used, the H-alpha line of the spectra was measured and 2-day normal values were formed in order to establish a temporal comparison. RESULTS: After the main maximum, during the period investigated by JD 2459292 to 2459305 at intervals of 2-5 weeks secondary maxima with different characteristics. The maxima of the equivalent width were 6-14 days after the respective brightness maxima. The maxima are interpreted as subsequent outbreaks of the nova. Possibly these are subsequent weaker eruptions of the nova or other mechanisms that lead to an increase in density in the envelope.