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researcher

M. Marley

339 papers hereh-index 8927.9k citations655 works total

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

author position
  • sole author3
  • first author18
  • middle author236
  • last author44

Across the 301 of 339 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP168
  • astro-ph.SR87
  • astro-ph65
  • astro-ph.IM14
  • astro-ph.GA5
same name
  • M. Marley — 19 papers, h 4

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
19962026
most citedA Non-Gray Theory of Extrasolar Giant Planets and Brown Dwarfs

1.4k citations · 31.2k across the 331 of their papers we have counts for

collaborators
Showing 2002Show all

4 papers · 1 filter

astro-ph2002

Clouds and Clearings in the Atmospheres of the L and T Dwarfs

M. S. Marley, A. Ackerman, A. J. Burgasser +3

A sophisticated approach to condensate opacity is required to properly model the atmospheres of L and T dwarfs. Here we review different models for the treatment of condensates in…

astro-ph2002

Non-equilibrium chemistry in the atmospheres of brown dwarfs

D. Saumon, M. S. Marley, K. Lodders +1

Carbon monoxide and ammonia have been detected in the spectrum of Gl 229B at abundances that differ substantially from those obtained from chemical equilibrium. Vertical mixing in…

astro-ph2002★ 159 cited

L-dwarf variability: I-band observations

Christopher R. Gelino, Mark S. Marley, Jon A. Holtzman +2

We report on the results of an I-band photometric variability survey of eighteen L dwarfs. We find that seven exhibit statistically significant variations above the 95.4% confidenc…

astro-ph2002★ 267 cited

Evidence for Cloud Disruption in the L/T Dwarf Transition

Adam J. Burgasser, Mark S. Marley, Andrew S. Ackerman +5

Clouds of metal-bearing condensates play a critical role in shaping the emergent spectral energy distributions of the coolest classes of low-mass stars and brown dwarfs, L and T dw…

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