Fundamental Physics with Brown Dwarfs: The Mass-Radius Relation

Bibcode
2019BAAS...51c.214B
Burgasser, Adam; Baraffe, Isabelle; Browning, Matthew; Burrows, Adam; Chabrier, Gilles; Creech-Eakman, Michelle; Demory, Brice; Dieterich, Sergio; Faherty, Jacqueline; Huber, Daniel; Lodieu, Nicolas; Plavchan, Peter; Rich, R. Michael; Saumon, Didier; Stassun, Keivan; Triaud, Amaury; van Belle, Gerard; van Grootel, Valerie; Vos, Johanna M.; Yadav, Rakesh
Bibliographical reference

Astro2020: Decadal Survey on Astronomy and Astrophysics, science white papers, no. 214; Bulletin of the American Astronomical Society, Vol. 51, Issue 3, id. 214 (2019)

Advertised on:
5
2019
Number of authors
20
IAC number of authors
1
Citations
0
Refereed citations
0
Description
The lowest-mass stars, brown dwarfs and giant exoplanets span a minimum in the mass-radius relationship that probes the fundamental physics of extreme states of matter, magnetism, and fusion. This White Paper outlines scientific opportunities and the necessary resources for modeling and measuring the mass- radius relationship in this regime.
Type
Non-refereed

It may interest you

  • Non-refereed
    Einasto Gravitational Potentials have Difficulty to Hold Spherically Symmetric Stellar Systems with Cores
    It was known that an ideal spherically symmetric stellar system with isotropic velocities and an inner core cannot reside in a Navarro, Frenk, and White (NFW) gravitational potential. The incompatibility can be pinned down to the radial gradient of the NFW potential in the very center of the system, which differs from zero. The gradient is
    Sánchez Almeida, Jorge

    Advertised on:

    6
    2024
    Bibcode
    2024RNAAS...8..167S
    Citations
    0
  • Non-refereed
    The Aligned Orbit of a Hot Jupiter around the M Dwarf TOI-4201
    Measuring the obliquities of stars hosting giant planets may shed light on the dynamical history of planetary systems. Significant efforts have been made to measure the obliquities of FGK stars with hot Jupiters, mainly based on observations of the Rossiter–McLaughlin effect. In contrast, M dwarfs with hot Jupiters have hardly been explored because
    Gan, Tianjun et al.

    Advertised on:

    7
    2024
    Bibcode
    2024ApJ...969L..24G
  • Non-refereed
    ROSALIA: ROman Sky Analyst for Low surface brightness Imaging & Astronomy
    Diffuse emission in the outskirts of galaxies, such as stellar tidal streams, galaxy stellar halos and intracluster light, provides important constraints on the structure and evolution of the Universe. However, such low surface brightness diffuse emission can be up to thousands of times dimmer (>29 AB mag/[square arcseconds]) than the sky
    Laine, Seppo et al.

    Advertised on:

    6
    2024
    Bibcode
    2024AAS...24412902L
    Citations
    0