The role of the synchrotron component in the mid-infrared spectrum of m 87

18Citations
Citations of this article
6Readers
Mendeley users who have this article in their library.

Abstract

We study in detail the mid-infrared (MIR) Spitzer-IRS spectrum of M 87 in the range 5-20 μm. Thanks to the high sensitivity of our Spitzer-IRS spectra we can disentangle the stellar and nuclear components of this active galaxy. To this end, we have properly subtracted from the M 87 spectrum the contribution of the underlying stellar continuum derived from passive Virgo galaxies in our sample. The residual is a clear power law, without any additional thermal component, with a zero-point consistent with that obtained by high spatial resolution, ground-based observations. The residual is independent of the adopted passive template. This indicates that the 10 μm silicate emission shown in the spectra of M 87 can be entirely accounted for by the underlying old stellar population, leaving little room for a possible torus contribution. The MIR power law has a slope α ∼0.77-0.82 (Sν ∝ ν -α), consistent with optically thin synchrotron emission.

Cite

CITATION STYLE

APA

Buson, L., Bressan, A., Panuzzo, P., Rampazzo, R., Valdes, J. R., Clemens, M., … Silva, L. (2009). The role of the synchrotron component in the mid-infrared spectrum of m 87. Astrophysical Journal, 705(1), 356–360. https://doi.org/10.1088/0004-637X/705/1/356

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free