HII regions in NGC 5457 and NGC 4395 (Cedres+, 2002)

Bibcode
2002yCat..33910809C
Cedres, B.; Cepa, J.
Referencia bibliográfica

VizieR On-line Data Catalog: J/A+A/391/809. Originally published in: 2002A&A...391..809C

Fecha de publicación:
5
2002
Número de autores
2
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
Line intensities, visual extinction, abundances and ionization hardness parameter for HII regions in two spiral galaxies are presented. The following galaxies have been observed: NGC 5457 and NGC 4395. In NGC 5457 have been obtained data for 338 regions. In NGC 4395 have been obtained data for 158 regions. For each region position, visual extinction, H-alpha flux, H-alpha equivalent width, H-beta flux, H-beta equivalent width, [OII] flux, [OIII] flux, [SII] flux, [SIII] flux (only for NGC 5457), R23 parameter, oxygen abundance and ionization hardness parameter (only for NGC 5457) are given. (6 data files).
Tipo
Sin árbitro
Regiones H II
Fotometría

Te puede interesar

  • Sin árbitro
    Estimation of the hydrostatic-to-lensing mass bias from resolved cluster masses
    We present a study on the bias of hydrostatic masses with respect to lensing mass estimates for a sample of 53 clusters in a redshift range between z = 0.05 and 1.07. The M 500 mass for each cluster was inferred from X-ray and lensing data, without using a priori observable-mass scaling relations. Cluster masses of our reference analysis were
    Muñoz-Echeverría, M. et al.

    Fecha de publicación:

    6
    2024
    Bibcode
    2024EPJWC.29300033M
    Número de citas
    0
  • Sin árbitro
    IRAM 30-meter millimeter follow-up of deep OSIRIS-GTC optical surveys
    It is broadly accepted that CO is a reliable tracer of H2 in massive IR (L IR ≳ 10 9 L ⊙) galaxies, and that there are clear correlations between L IR and L' CO that are qualitatively independent of environment and even redshift. We present two tales on the search for 12CO emission from dusty star-forming galaxies in both field (Lockman Hole, z < 0
    Sánchez-Portal, M. et al.

    Fecha de publicación:

    6
    2024
    Bibcode
    2024EPJWC.29300047S
    Número de citas
    0
  • Sin árbitro
    The NIKA2 Sunyaev-Zeldovich Large Program. Sample and upcoming product public release
    The NIKA2 camera operating at the IRAM 30-m telescope excels in high-angular resolution mapping of the thermal Sunyaev-Zel'dovich effect towards galaxy clusters at intermediate and high-redshift. As part of the NIKA2 guaranteed-time, the SZ Large Program (LPSZ) aims at tSZ-mapping a representative sample of SZ-selected galaxy clusters in the
    Perotto, L. et al.

    Fecha de publicación:

    6
    2024
    Bibcode
    2024EPJWC.29300040P
    Número de citas
    0