Pith. sign in

REVIEW

The L to T Dwarf Transition

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv astro-ph/0409267 v1 pith:26SERH6P submitted 2004-09-10 astro-ph

classification astro-ph
keywords transitioncloudchangingatmosphericdecksdwarfdynamicsacceptable
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

While the precise mechanism responsible for the L to T dwarf transition remains unclear, it is clearly caused by changing cloud characteristics. Here we briefly review data relevant to understanding the nature of the transition and argue that changing atmospheric dynamics produce the transition by opening holes through the global iron and silicate cloud decks. Other possibilities, such as a sudden vertical collapse in these cloud decks are also considered. Any acceptable model of the L to T transition must ultimately connect changing cloud properties to the underlying atmospheric dynamics.

Discussion (0). Sign in to comment.

Pith tools