New Physics and Features in the 2.2 Release of the PHOEBE Eclipsing Binary Modeling Code

Bibcode
2020AAS...23511405C
Conroy, K.; Jones, D.; Horvat, M.; Pablo, H.; Kochoska, A.; Giammarco, J.; Prsa, A.
Bibliographical reference

American Astronomical Society Meeting Abstracts

Advertised on:
1
2020
Number of authors
7
IAC number of authors
1
Citations
1
Refereed citations
1
Description
PHOEBE (phoebe-project.org) is a sophisticated code for modeling eclipsing binary observables. PHOEBE 2.0 (Prsa et al, 2016) introduced increased precision, triangulated meshing, light travel time effects, Doppler boosting, improved atmospheric and passband treatments, and a Python frontend interface. PHOEBE 2.1 (Horvat et al, 2018) added support for misalignment, synthetic spectral line profiles, and a re-parameterization from equipotentials and polar radii to equivalent radii. In the 2.2 release, we now introduce interstellar extinction, additional passband scaling options including color-support, advanced third light and limb-darkening, and support for Python 3.
Type
Non-refereed

It may interest you

  • Non-refereed
    The luminosity functions of an homogeneous sample of 50 young nearby open clusters
    Open clusters are groups of coeval stars sharing properties such as distance and metallicity, and they are key to understanding stellar evolution. We shed light on the evolution of open clusters with a special focus on the universality of the luminosity function. We applied an upgraded version of the convergent point technique on about 50 open
    Lodieu, Nicolas et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf..512L
    Citations
    0
  • Non-refereed
    Gas Flows in the Central Regions of NGC 4593 with Muse
    Gas flows into the centres of galaxies form an important ingredient to the formation, growth and evolution of galaxies. The process of gas falling into the central supermassive black hole (SMBH) can lead to high levels of non-stellar emission which results in an active galactic nucleus (AGN). However, the details of how such gas flows reach the
    Mulumba, Dorcus et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf..479M
    Citations
    0
  • Non-refereed
    The effect of local and large scale environment on star formation histories in galaxies
    The environment of galaxies plays a key role in their evolution. The availability of large extragalactic surveys makes it possible to place a galaxy not only in its immediate environment, but also in its position within the large-scale structure of the universe. Within this context, we investigate how the local environment influences the star
    Torres-Ríos, Gloria et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf.1965T
    Citations
    0