The dolmens and "Hawanat" of Africa Proconsularis revisited

Bibcode
2003JHA....34..305B
Belmonte, J. A.; Perera Betancort, M. A. ; Marrero, Rita; Gaspar, Antonio Tejera
Bibliographical reference

Journal for the History of Astronomy (ISSN 0021-8286), Vol. 34, Part 3, No. 116, p. 305 - 320 (2003)

Advertised on:
8
2003
Number of authors
4
IAC number of authors
1
Citations
0
Refereed citations
0
Description
Not Available
Type
Refereed

It may interest you

  • Refereed
    MUSE view of PDS 456: Kiloparsec-scale wind, extended ionized gas, and close environment
    PDS 456 is the most luminous (L bol ∼ 10 47 erg s −1) radio-quiet quasar at z < 0.3 and can be regarded as a local counterpart of the powerful quasars shining at Cosmic Noon. It hosts a strong nuclear X-ray ultra-fast (∼0.3c) outflow, and a massive and clumpy CO (3-2) molecular outflow extending up to ∼5 kpc from the nucleus. We analyzed the first
    Travascio, A. et al.

    Advertised on:

    6
    2024
    Bibcode
    2024A&A...686A.250T
    Citations
    0
  • Refereed
    TOI-837 b is a young Saturn-sized exoplanet with a massive 70 M<SUB>⊕</SUB> core
    We present an exhaustive photometric and spectroscopic analysis of TOI-837, a F9/G0 35 Myr young star, hosting a transiting exoplanet, TOI-837 b, with an orbital period of ~8.32 d. Utilizing data from the Transiting Exoplanet Survey Satellite and ground-based observations, we determine a planetary radius of $0.818_{-0.024}^{+0.034}$ R J for TOI-837
    Barragán, Oscar et al.

    Advertised on:

    7
    2024
    Bibcode
    2024MNRAS.531.4275B
    Citations
    0
  • Refereed
    Changing Look of the Optical Spectrum of the MeV Blazar PKS 0446+112 (4FGL J0449.1+1121)
    Following the high activity of the γ-ray Fermi source 4FGL J0449.1+1121 (PKS 0446+112), possibly associated with a IceCube neutrino event IC-240105A, we obtained optical spectroscopy with the Gran Telescopio Canarias of the counterpart. We detect a clear emission line at 3830 Å identified as Lyα that confirms the redshift of source at z = 2.153
    Paiano, Simona et al.

    Advertised on:

    6
    2024
    Bibcode
    2024ApJ...968...81P
    Citations
    0