Zobrazeno 1 - 10
of 14
pro vyhledávání: '"L. M. Cairós"'
(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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e0f874f06c9354f4345cca7d84f1e06c
Autor:
J. N. González-Pérez, L. M. Cairós
(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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cd5d2326e335b50998ab8882b4dc3881
Autor:
J. N. González-Pérez, L. M. Cairós
(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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::94d0ee000a28976df71fe32ac8ebec72
http://arxiv.org/abs/1708.09407
http://arxiv.org/abs/1708.09407
Autor:
Martin Roth, Nicola Caon, Polychronis Papaderos, Peter M. Weilbacher, L. M. Cairós, C. Zurita, Carolina Kehrig
Publikováno v:
The Astrophysical Journal. 707:1676-1690
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::df35e15f3aacf2db814aa565a967cd72
https://doi.org/10.1088/0004-637x/707/2/1676
https://doi.org/10.1088/0004-637x/707/2/1676
Publikováno v:
Astronomy & Astrophysics. 507:1291-1301
(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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::eaba99665e21c1f5b304dea2379129a2
https://doi.org/10.1051/0004-6361/200811576
https://doi.org/10.1051/0004-6361/200811576
Publikováno v:
The Astrophysical Journal. 677:201-218
We present results on integral-field optical spectroscopy of five luminous Blue Compact Dwarf galaxies. The data were obtained using the fiber system INTEGRAL attached at the William Herschel telescope. The galaxies Mrk 370, Mrk 35, Mrk 297, Mrk 314
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3486cfb0bff1667b69c6cb696f555c9b
https://doi.org/10.1086/528785
https://doi.org/10.1086/528785
Publikováno v:
The Astrophysical Journal. 577:164-182
We present results from a detailed spectrophotometric analysis of the blue compact dwarf galaxy (BCD) Mrk 370, based on deep UBVRI broad-band and Halpha narrow-band observations, and long-slit and two-dimensional spectroscopy of its brightest knots.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6f4b8b19821844d435f92261e0bfde62
https://doi.org/10.1086/342134
https://doi.org/10.1086/342134
Autor:
L. M. Cairós, J. N. González-Pérez
Publikováno v:
Astronomy & Astrophysics. 600:A125
(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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2c5e1cce2a13eea7acba43578a428003
https://doi.org/10.1051/0004-6361/201629681
https://doi.org/10.1051/0004-6361/201629681
Publikováno v:
The Astrophysical Journal Supplement Series. 136:393-416
This is the second in a series of papers devoted to the study of a sample of 28 blue compact dwarf galaxies (BCDs). In the first paper, we presented the broadband observations in B, V, R, and I. Deep contour maps, surface-brightness profiles, and col
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::246e3bc98ddeb594df6a48a6965b2959
https://doi.org/10.1086/322532
https://doi.org/10.1086/322532
Publikováno v:
Astrophysics and Space Science Proceedings ISBN: 9783642220173
Blue Compact Dwarf (BCD) galaxies are metal-poor and gas-rich systems undergoing intense, spatially extended star-forming activity. These galaxies offer a unique opportunity to investigate dwarf galaxy formation and evolution, and probe violent star
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6a83a3f3ba9a60136c63d6e55afa086a
https://doi.org/10.1007/978-3-642-22018-0_24
https://doi.org/10.1007/978-3-642-22018-0_24