Zobrazeno 1 - 10
of 40
pro vyhledávání: '"Cairos, L. M."'
Publikováno v:
A&A 664, A144 (2022)
We investigate the warm ionized gas in the blue compact galaxy (BCG) Haro 14 by means of integral field spectroscopic observations taken with the MUSE/VLT. The large FoV of MUSE and its unprecedented sensitivity enable observations of the galaxy nebu
Externí odkaz:
http://arxiv.org/abs/2206.02754
Publikováno v:
A&A 654, A142 (2021)
(Abriged) Blue compact galaxies (BCGs) are low-luminosity, metal-poor, gas-rich objects that form stars at high rates, excellent analogs to the high-redshift star-forming galaxy population. Being low-mass starbursts, they also constitute ideal labora
Externí odkaz:
http://arxiv.org/abs/2108.09107
Autor:
Cairós, L. M., González-Pérez, J. N.
Publikováno v:
A&A 634, A95 (2020)
(Abridged) Low-luminosity, active star-forming blue compact galaxies (BCGs) are excellent laboratories for investigating the process of star formation on galactic scales and probing the interplay between massive stars and the surrounding interstellar
Externí odkaz:
http://arxiv.org/abs/2001.02573
Autor:
Cairós, L. M., González-Pérez, J. N.
Publikováno v:
A&A 608, A119 (2017)
(Abridged) Blue compact galaxies (BCG) are gas-rich, low-mass, small systems that form stars at unusually high rates. This makes them excellent laboratories for investigating the process of star-formation (SF) at galactic scales and the effects of ma
Externí odkaz:
http://arxiv.org/abs/1708.09407
Autor:
Cairós, L. M., González-Pérez, J. N.
Publikováno v:
A&A 600, A125 (2017)
(Abridged) Low-luminosity, gas-rich blue compact galaxies (BCG) are ideal laboratories to investigate many aspects of the star formation in galaxies. We study the morphology, stellar content, kinematics, and the nebular excitation and ionization mech
Externí odkaz:
http://arxiv.org/abs/1703.04672
Autor:
Cairos, L. M., Caon, N., Garcia-Lorenzo, B., Kelz, A., Roth, M., Papaderos, P., Streicher, O.
[abridged] We carry out an integral field spectroscopy (IFS) study of a sample of luminous BCGs, with the aim to probe the morphology, kinematics, dust extinction and excitation mechanisms of their warm interstellar medium (ISM). IFS data for five lu
Externí odkaz:
http://arxiv.org/abs/1209.0310
(Abridged) We perform integral field spectroscopy of a sample of Blue compact dwarf (BCD) galaxies with the aim of analyzing their morphology, the spatial distribution of some of their physical properties (excitation, extinction, and electron density
Externí odkaz:
http://arxiv.org/abs/1004.2858
Publikováno v:
Astrophys.J.707:1676-1690,2009
We present an integral field spectroscopic study of the central 2x2 kpc^2 of the blue compact dwarf galaxy Mrk 409, observed with the Potsdam MultiAperture Spectrophotometer. This study focuses on the morphology, two-dimensional chemical abundance pa
Externí odkaz:
http://arxiv.org/abs/0911.2344
(Abridged) Aims: By means of optical Integral Field Spectroscopy (IFS) observations, we aim to disentangle and characterize the starburst component in the BCD Mrk 1418. In particular we propose to study the stellar and ionized gas morphology, to inve
Externí odkaz:
http://arxiv.org/abs/0908.1305
We have characterized the underlying stellar host in a sample of 28 blue compact galaxies (BCGs), by fitting their 2D light distributions. Their structural parameters were related with galaxy properties such as colours and gas content. These properti
Externí odkaz:
http://arxiv.org/abs/0903.2861