The spectrum and evolution of compact SNR: SN and AGN.

Bibcode
1993RMxAA..27..133F
Tenorio-Tagle, G.; Rosz˙Yczka, M.; Terlevich, R.; Cox, D.; Miller, W.; Franco, J.
Bibliographical reference

Revista Mexicana de Astronomia y Astrofisica, Vol. 27, p. 133 - 136

Advertised on:
11
1993
Journal
Revista Mexicana de Astronomía y Astrofísica
Number of authors
6
IAC number of authors
1
Citations
15
Refereed citations
11
Description
The evolution and spectra from a compact supernova remnant evolving in a high-density circumstellar medium with a density of 107cm-3 are presented. The radiation emitted by the shocked region can self-ionize the cooling shell and a large region of the surrounding medium. The resulting line ratios from the photoionized zones are similar to those observed in active galactic nuclei.
Type
Refereed
Supernova remnants
Active galactic nuclei

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
    CEERS Key Paper. IX. Identifying Galaxy Mergers in CEERS NIRCam Images Using Random Forests and Convolutional Neural Networks
    A crucial yet challenging task in galaxy evolution studies is the identification of distant merging galaxies, a task that suffers from a variety of issues ranging from telescope sensitivities and limitations to the inherently chaotic morphologies of young galaxies. In this paper, we use random forests and convolutional neural networks to identify
    Rose, Caitlin et al.

    Advertised on:

    11
    2024
    Bibcode
    2024ApJ...976L...8R
    Citations
    0
  • Refereed
    Distance estimation of gamma-ray-emitting BL Lac objects from imaging observations
    Aims. The direct redshift determination of BL Lac objects is highly challenging as the emission in the optical and near-infrared bands is largely dominated by the non-thermal emission from the relativistic jet, which points very close to our line of sight. Therefore, the optical spectra of BL Lac objects often show no spectral lines from the host
    Nilsson, K. et al.

    Advertised on:

    11
    2024
    Bibcode
    2024A&A...691A.154N
    Citations
    0