Stellar population in bulge of spiral galaxies

Bibcode
2007NCimB.122.1281M
DOI
10.1393/ncb/i2008-10492-y
Morelli, L.; Pompei, E.; Pizzella, A.; Coccato, L.; Corsini, E. M.; Méndez-Abreu, J.; Saglia, R. P.; Sarzi, M.; Bertola, F.
Bibliographical reference

Il Nuovo Cimento B, vol. 122, Issue 9, p.1281-1284

Advertised on:
9
2007
Number of authors
9
IAC number of authors
0
Citations
1
Refereed citations
1
Description
We present a preliminary analysis of ASTRO-F data of a complete sample of ~150 EROs (R-K>5) down to K(Vega)<19, for which reliable photometric redshifts are available, in the range 0.8
Type
Refereed

It may interest you

  • Refereed
    The size-luminosity relation of local active galactic nuclei from interferometric observations of the broad-line region
    By using the GRAVITY instrument with the near-infrared (NIR) Very Large Telescope Interferometer (VLTI), the structure of the broad (emission-)line region (BLR) in active galactic nuclei (AGNs) can be spatially resolved, allowing the central black hole (BH) mass to be determined. This work reports new NIR VLTI/GRAVITY interferometric spectra for
    GRAVITY Collaboration et al.

    Advertised on:

    4
    2024
    Bibcode
    2024A&A...684A.167G
    Citations
    8
  • Refereed
    A dusty protocluster surrounding the binary galaxy HerBS-70 at z = 2.3
    We report on deep SCUBA-2 observations at 850 $\mu$m and NOrthern Extended Millimetre Array (NOEMA) spectroscopic measurements at 2 mm of the environment surrounding the luminous, massive (M * ≈ 2 × 10 11 M ⊙) Herschel-selected source HerBS-70. This source was revealed by previous NOEMA observations to be a binary system of dusty star-forming
    Bakx, Tom J. L. C. et al.

    Advertised on:

    6
    2024
    Bibcode
    2024MNRAS.530.4578B
    Citations
    0
  • Refereed
    Overmassive Black Holes at Cosmic Noon: Linking the Local and the High-redshift Universe
    We report for the first time a sample of 12 supermassive black holes (SMBHs) hosted by low-mass galaxies at cosmic noon, i.e., in a redshift range consistent with the peak of star formation history: z ∼ 1–3. These black holes are 2 orders of magnitude too massive for the stellar content of their hosts when compared with the local relation for
    Mezcua, Mar et al.

    Advertised on:

    5
    2024
    Bibcode
    2024ApJ...966L..30M
    Citations
    0