pea galaxy

Pea galaxies have a strong emission line when compared to the rest of their spectral continuum.

Pea galaxies are among the most active star-forming galaxies ever found.

Cardamone et al. describe Pea galaxies as having a low metallicity, but that the oxygen present is highly ionized.

Pea galaxies are rare.

Comparing a Pea galaxy to the Milky Way can be useful when trying to visualize these star-forming rates.

These "Pea galaxies" appear in the SDSS as unresolved green images.

However, for the hottest Green Pea galaxies, which appear to be dwarf galaxies, this explanation does not seem to be plausible.

To date only five Pea galaxies have been imaged by the Hubble Space Telescope (HST).

Pea galaxies have low interstellar reddening values, as shown in the histogram on the right, with nearly all Peas having E(B-V) 0.25.

Pea galaxies (Pea galaxies) are small compact galaxies resembling primordial starbursts.

Pea galaxies exist at a time when the Universe was three-quarters of its present age and so are clues as to how galaxy formation took place in the earlier Universe.

Pea galaxies are so-named because of their small size and greenish appearance in the images taken by the Sloan Digital Sky Survey (SDSS).

The imaging and spectroscopy for the three Green Pea galaxies was carried out using the OSIRIS instrument mounted on the GTC 10.4m telescope.

One of the original ways of recognizing Pea galaxies, before SQL programming was involved, was because of a discrepancy about how the SDSS labels them within Skyserver.

A Pea galaxy, also referred to as a Pea or Green Pea, might be a type of Luminous Blue Compact Galaxy which is undergoing very high rates of star formation.