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Kelly Lepo
@kellylepo.bsky.social
Astronomer | Science communicator | Adult Lisa Simpson Education and Outreach Scientist at the Space Telescope Science Institute (@spacetelescope.bsky.social) supporting JWST. Personal account — Views are my own Also on Mastodon: @kellylepo@astrodon.social
1.2k followers153 following542 posts

KLkellylepo.bsky.social

First session: The Powerful Shocks in Novae V: Revisiting Novae with a Multi-messenger Approach Kirill Sokolovsky: NuSTAR observations of classical novae show depleted iron (or enhanced CNO). X-ray light curves don't have periodic changes like in visible light -> X-rays are made further out #AAS244

NuSTAR lightcurves and shock location
• Some variability on ~10 hour timescale
• No periodic modulation (orbital/WD rotation)
• No obvious correlation with optical
Shocked region is large compared to the binary?
Not directly related to optical - below the photosphere?
Summary
• NuSTAR spectra of all detected novae look alike
• Consistent with single-temperature CNO-enriched plasma
• Heavily absorbed - shocks are deep within ejecta
• But no fast variability, so not too close to the WD
Lx/Ly <<1, defying explanation
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KL
Kelly Lepo
@kellylepo.bsky.social
Astronomer | Science communicator | Adult Lisa Simpson Education and Outreach Scientist at the Space Telescope Science Institute (@spacetelescope.bsky.social) supporting JWST. Personal account — Views are my own Also on Mastodon: @kellylepo@astrodon.social
1.2k followers153 following542 posts