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pro vyhledávání: '"Garland C"'
Luminous compact blue galaxies (LCBGs) have enhanced star formation rates and compact morphologies. We combine Sloan Digital Sky Survey data with HI data of 29 LCBGs at redshift z~0 to understand their nature. We find that local LCBGs have high atomi
Externí odkaz:
http://arxiv.org/abs/1506.04649
Autor:
Rabidoux, Katie, Pisano, D. J., Garland, C. A., Guzman, Rafael, Castander, Francisco J., Wolfe, Spencer
While bright, blue, compact galaxies are common at $\rm z \sim 1$, they are relatively rare in the local universe, and their evolutionary paths are uncertain. We have obtained resolved H I observations of nine $\rm z \sim 0$ luminous compact blue gal
Externí odkaz:
http://arxiv.org/abs/1412.4739
Autor:
Pérez-Gallego, J., Guzmán, R., Castillo-Morales, A., Gallego, J., Castander, F. J., Garland, C. A., Gruel, N., Pisano, D. J., Zamorano, J.
We use three dimensional optical spectroscopy observations of a sample of 22 local Luminous Compact Blue Galaxies (LCBGs) to create kinematic maps. By means of these, we classify the kinematics of these galaxies into three different classes: rotating
Externí odkaz:
http://arxiv.org/abs/1108.2994
High-resolution X-ray scattering studies of the nonpolar thermotropic liquid crystal 4-n-pentylphenylthiol-4'-n-octyloxybenzoate (\bar{8}S5) in aerosil gel nano-networks reveal that the aerosil-induced disorder significantly alters both the nematic t
Externí odkaz:
http://arxiv.org/abs/1104.5670
Luminous compact blue galaxies (LCBGs) are a diverse class of galaxies characterized by high luminosity, blue color, and high surface brightness that sit at the critical juncture of galaxies evolving from the blue to the red sequence. As part of our
Externí odkaz:
http://arxiv.org/abs/1101.3290
Autor:
Pisano, D. J., Garland, C., Rabidoux, K., Wolfe, S., Guzman, R., Perez-Gallego, J., Castander, F. J.
Publikováno v:
AIP Conf.Proc.1240:119-122,2010
Luminous compact blue galaxies (LCBGs) are a diverse class of galaxies characterized by high luminosities, blue colors, and high surface brightnesses. Residing at the high luminosity, high mass end of the blue sequence, LCBGs sit at the critical junc
Externí odkaz:
http://arxiv.org/abs/0912.3283
Autor:
Pérez-Gallego, J., Guzmán, R., Castillo-Morales, A., Castander, F. J., Gallego, J., Garland, C. A., Gruel, N., Pisano, D. J., Sánchez, S. F., Zamorano, J.
The kinematic properties of the ionized gas of local Luminous Compact Blue Galaxy (LCBG) NGC 7673 are presented using three dimensional data taken with the PPAK integral field unit at the 3.5-m telescope in the Centro Astron\'omico Hispano Alem\'an.
Externí odkaz:
http://arxiv.org/abs/0911.1069
Luminous Compact Blue Galaxies (LCBGs) are common at z~1, contributing significantly to the total star formation rate density. By z~0, they are a factor of ten rarer. While we know that LCBGs evolve rapidly, we do not know what drives their evolution
Externí odkaz:
http://arxiv.org/abs/0712.1243
We have studied the effects of quenched random disorder created by dispersed aerosil nanoparticle gels on the nematic to smectic-A (N-SmA) and smectic-A to reentrant nematic (SmA- RN) phase transitions of thermotropic liquid crystal mixtures of 6OCB
Externí odkaz:
http://arxiv.org/abs/0711.2763