Discovery of Multiple High-Velocity Narrow Circumstellar Na I D Lines in Nova V1280 Sco
Kozo Sadakane, Akito Tajitsu, Sahori Mizoguchi, Akira Arai, Hiroyuki, Naito

TL;DR
This study reports the discovery of multiple high-velocity, narrow Na I D absorption lines in Nova V1280 Sco, indicating cool clumpy circumstellar gas interactions, with detailed spectral analysis over two months.
Contribution
First detection of multiple high-velocity narrow Na I D absorption components in Nova V1280 Sco, revealing complex circumstellar gas dynamics post-explosion.
Findings
Discovered at least 11 distinct Na I D absorption components.
High-velocity components remained nearly constant in wavelength over two months.
Na I D lines showed narrow, deepening absorption features, unlike Fe II and Balmer lines.
Abstract
We discovered multiple high-velocity (ranging from -900 to -650 km/s) and narrow (FWHM = 15 km/s) absorption components corresponding to both the D2 and the D1 lines of Na I on a high dispersion spectrum of V1280 Sco observed on 2009 May 9 (UT), 814 d after the V-band maximum. Subsequent observations carried out on 2009 June and July confirmed at least 11 distinct absorption components in both systems. Some components had deepened during the two months period while their HWHMs and wavelengths remained nearly constant. We suggest these high velocity components originate in cool clumpy gas clouds moving on the line of sight, produced in interactions between pre-existing cool circumstellar gas and high velocity gas ejected in the nova explosion. The optical region spectrum of V1280 Sco in 2009 is dominated by the continuum radiation and exhibits no forbidden line characterizing the nebular…
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