The Problem of English as a Foreign Language in Professional Astronomy

Bibcode
2000ASSL..256..185M
Mahoney, T. J.
Bibliographical reference

Organizations and Strategies in Astronomy. Edited by André Heck; Observatoire Astronomique, Strasbourg, France Astrophysics and Space Science Library, Volume 256 Kluwer Academic Publishers, Volume 256. Kluwer Academic Publishers, Dordrecht, 2000, p.185

Advertised on:
11
2000
Number of authors
1
IAC number of authors
1
Citations
2
Refereed citations
2
Description
Not Available
Type
Non-refereed

It may interest you

  • Non-refereed
    A Disc Wind Where You Least Expect It: The Outflow in the Short-period X-ray Binary UW CrB
    Studying outflows of low mass X-ray binaries (LMXBs) is important for understanding the physics of accretion, the evolution of compact binaries, and dynamics of the local interstellar medium. One significant source of these outflows is the accretion disc wind, which can blow away vast amounts of material from the disc before it can be accreted on
    Fijma, Stefanie et al.

    Advertised on:

    5
    2024
    Bibcode
    2024HEAD...2150106F
    Citations
    0
  • Non-refereed
    Rapid multiwavelength variability reveals jet emission in the black hole binary V404 Cygni in quiescence
    Spitzer Space Telescope observations of several quiescent black hole low mass X-ray binaries (LMXBs) have shown mid-infrared excesses above the emission of a companion star. The excess has been proposed to originate from either a relativistic jet or circumbinary disk. If the mid-IR originates in a jet, then it probes the region closest to the black
    Borowski, Eric et al.

    Advertised on:

    5
    2024
    Bibcode
    2024HEAD...2130105B
    Citations
    0
  • Non-refereed
    Application of Bayesian Inference to disentangle CMB foregrounds
    Both Galactic dust emission and Cosmic infrared background anisotropies (CIB) act as a dominant foreground contaminant for the measurements of the CMB anisotropies (intensity and polarization) at the frequency range above 217 GHz. The Galactic dust and CIB share a similar form of spectral energy distribution, which makes it harder to disentangle
    Adak, Debabrata et al.

    Advertised on:

    1
    2024
    Bibcode
    2024asi..confP..71A
    Citations
    0