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researcher

Masaki Takayama

3 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author1
  • first author1
  • middle author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
same name
  • Masaki Takayama — 1 paper, h 1

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20152024
most citedProbable detection of an eruptive filament from a superflare on a solar-type star

144 citations · 159 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2024

Period modulations of the long secondary periods on the AGB stars

Masaki Takayama

30%--50% of the luminous pulsating red-giant stars show light variations of a longer period than the pulsation periods. Those periods are called long secondary periods (LSP).…

astro-ph.SR2021★ 144 cited

Probable detection of an eruptive filament from a superflare on a solar-type star

Kosuke Namekata, Hiroyuki Maehara, Satoshi Honda +20

Solar flares are often accompanied by filament/prominence eruptions (∼104 K and ∼1010−11 cm−3), sometimes leading to coronal mass ejections (CMEs) that direct…

astro-ph.SR2015★ 15 cited

Using broadband photometry to examine the nature of Long Secondary Periods in red giants

M. Takayama, P. R. Wood, Y. Ita

Long-term JHK light curves have recently become available for large numbers of the more luminous stars in the SMC. We have used these JHK light curves, along with OGLE V and…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.