Structure and Evolution of Circumstellar Shells Formed by Massive Star Winds

Bibcode
1995Ap&SS.224..459G
DOI
10.1007/BF00667904
García-Segura, Guillermo; Mac Low, Mordecai-Mark; Langer, Norbert
Bibliographical reference

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 459-460

Advertised on:
2
1995
Journal
Astrophysics and Space Science
Number of authors
3
IAC number of authors
1
Citations
0
Refereed citations
0
Description
We follow the interaction of massive stars with their circumstellar gas over their entire life-times by combining hydrodynamic stellar evolution calculations for 35 and 60M &sun; stars and one- and two-dimensional gas dynamical calculations for the circumstellar medium.
Type
Refereed

It may interest you

  • Refereed
    An ultra-short-period super-Earth with an extremely high density and an outer companion
    We present the discovery and characterization of a new multi-planetary system around the Sun-like star K2-360 (EPIC 201595106). K2-360 was first identified in K2 photometry as the host of an ultra-short-period (USP) planet candidate with a period of 0.88 d. We obtained follow-up transit photometry, confirming the star as the host of the signal
    Livingston, John H. et al.

    Advertised on:

    11
    2024
    Bibcode
    2024NatSR..1427219L
    Citations
    0
  • Refereed
    CAVITY: Calar Alto Void Integral-field Treasury surveY: I. First public data release
    The Calar Alto Void Integral-field Treasury surveY (CAVITY) is a legacy project aimed at characterising the population of galaxies inhabiting voids, which are the most under-dense regions of the cosmic web, located in the Local Universe. This paper describes the first public data release (DR1) of CAVITY, comprising science-grade optical data cubes
    García-Benito, Rubén et al.

    Advertised on:

    11
    2024
    Bibcode
    2024A&A...691A.161G
    Citations
    0
  • Refereed
    BOWIE-ALIGN: A JWST comparative survey of aligned versus misaligned hot Jupiters to test the dependence of atmospheric composition on migration history
    A primary objective of exoplanet atmosphere characterization is to learn about planet formation and evolution, however, this is challenged by degeneracies. To determine whether differences in atmospheric composition can be reliably traced to differences in evolution, we are undertaking a transmission spectroscopy survey with JWST to compare the
    Kirk, James et al.

    Advertised on:

    1
    2024
    Bibcode
    2024RASTI...3..691K
    Citations
    1