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AME in LDN 1780

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Diffuse Radio Foregrounds

Part of the book series: Springer Theses ((Springer Theses))

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Abstract

In this chapter we study the AME in the Lynds Dark Nebula (LDN) 1780 . Here, we have detected AME using interferometric observations at 31 GHz with 6\(^\prime \) angular resolution (Vidal et al. 2011).

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Notes

  1. 1.

    The extinction at a particular wavelength, in this case at the location of the H\(\alpha \) line at 656.3 nm, can be estimated from the extinction in the V band using the extinction curve. The extinction at the V band A(V) is related with the reddening \(E(B-V)\) through: \(A(V)/E(B-V)=R(V)\), with R(V) having a typical value of 3.1 in the Milky way.

  2. 2.

    http://lambda.gsfc.nasa.gov/.

  3. 3.

    http://www.sciops.esa.int/index.php?project=planck&page=Planck_Legacy_Archive.

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Authors and Affiliations

  1. Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester, UK

    Matías Vidal Navarro

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  1. Matías Vidal Navarro
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Correspondence to Matías Vidal Navarro .

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Vidal Navarro, M. (2016). AME in LDN 1780. In: Diffuse Radio Foregrounds. Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-319-26263-5_5

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