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M. Lewis

4 papers hereh-index 562 citations22 works total

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

author position
  • first author1
  • middle author2
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
  • astro-ph.GA1
same name
  • M. Lewis — 5 papers, h 1
  • M. Lewis — 3 papers, h 1
  • M. Lewis — 3 papers, h 2
  • M. Lewis — 2 papers, h 3
  • M. Lewis — 2 papers, h 2
  • M. Lewis — 1 paper, h 7

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

collaborators

4 papers

astro-ph.SR2026

29SiO and 30SiO J=1--0 maser signatures in Galactic AGB stars: the impact of third dredge up and turbulence velocity

M. O. Lewis, L. O. Sjouwerman, Y. M. Pihlström +3

J=1--0 SiO masers at 43 GHz have a well-established distinctive signature in asymptotic giant branch (AGB) stars. 28SiO transitions typically dominate these spectra with the v=1 an…

astro-ph.SR2026

ATOMIUM: Inner circumstellar envelopes of oxygen-rich AGB stars as revealed by highly excited SiO lines

B. Pimpanuwat, S. Etoka, M. D. Gray +14

Silicon monoxide (SiO) traces the physical conditions and dynamics in the circumstellar envelopes (CSEs) of AGB stars. We present high-resolution ALMA Band 6 observations of highly…

astro-ph.SR2024

Classification of Wolf Rayet stars using Ensemble-based Machine Learning algorithms

Subhajit Kar, Rajorshi Bhattacharya, Ramkrishna Das +2

We develop a robust Machine Learning classifier model utilizing the eXtreme-Gradient Boosting (XGB) algorithm for improved classification of Galactic Wolf-Rayet (WR) stars based on…

astro-ph.GA2024

The Milky Way bar potential constrained by the kinematics of SiO maser stars in BAaDE Survey

Tian-Ye Xia, Juntai Shen, Zhi Li +5

We introduce a novel method that utilizes the longitude-velocity (l-v) envelope to constrain the Milky Way (MW) bar potential. Previous work (Habing 2016) used the l-v diagram to e…

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