Resolving the Mid- and Far-IR Emission of Seyfert Galaxies

Bibcode
2001ASPC..249..302A
Acosta-Pulido, J. A.; González Hernández, J. I.; Pérez García, A. M.; Rodríguez Espinosa, J. M.
Bibliographical reference

The Central Kiloparsec of Starbursts and AGN: The La Palma Connection, ASP Conference Proceedings Vol. 249. Edited by J. H. Knapen, J. E. Beckman, I. Shlosman, and T. J. Mahoney. ISBN: 1-58381-089-7. San Francisco: Astronomical Society of the Pacific, 2001, p. 302.

Advertised on:
0
2001
Number of authors
4
IAC number of authors
4
Citations
1
Refereed citations
1
Description
We present mid- and far-IR data from the CfA Seyfert sample, obtained with two instruments---ISOCAM and ISOPHOT---on board ISO. The spatial resolution of ISOCAM images allows us to separate the nuclear and extended contributions of the integrated emission. The improved spatial resolution of the ISOPHOT detectors allows us for the first time to provide ``nuclear'' photometry in the far IR for some galaxies. We also study the correlation between the mid-IR emission (nuclear and integrated) with the photometric data from 16 to 120 microns (ISOPHOT data).
Type
Non-refereed

It may interest you

  • Non-refereed
    Tales of stellar & binary co-evolution, told by stellar oscillations
    Stellar binarity and stellar oscillations are mostly seen and studied as two separate phenomena. Sometimes, one process is even complicating the analysis of the other beyond the liking of one or the other research community. However, the complete picture painted by the physical constraints provided by the combination of both processes represents a
    Beck, Paul G.

    Advertised on:

    10
    2024
    Bibcode
    2024bss..confE..35B
    Citations
    0
  • Non-refereed
    Convection, rotation, and magnetic activity of solar-like stars from asteroseismology
    During the last decade, our understanding of stellar physics and evolution has undergone a tremendous revolution thanks to asteroseismology. Space missions such as CoRoT, Kepler, K2, and TESS have already been observing millions of stars providing high-precision photometric data. With these data, it is possible to study the convection of stars
    Mathur, Savita

    Advertised on:

    0
    2024
    Bibcode
    2024IAUS..365..195M
    Citations
    0
  • Non-refereed
    The Multimodal Universe: 100 TB of Machine Learning Ready Astronomical Data
    We present the Multimodal Universe, a new framework collating over 100 TB of multimodal astronomical data for its first release, spanning images, spectra, time series, tabular and hyper-spectral data. This unified collection enables a wide variety of machine learning (ML) applications and research across astronomical domains. The dataset brings
    Angeloudi, Eirini et al.

    Advertised on:

    12
    2024
    Bibcode
    2024RNAAS...8..301A
    Citations
    0