On the Nature of the Faint Compact Narrow Emission-Line Galaxies: The Half-Light Radius–Velocity Width Diagram

Abstract

We present new measurements of emission-line velocity widths for five faint compact narrow emission-line galaxies (CNELGs) with 20.5 #B #21.5 and redshifts z10.19 to 0.35. The spectra were taken at the Keck telescope using the HIRES spectrograph with a resolution of 8 km s 21 (FWHM). Emission-line profiles are roughly Gaussian with velocity widths s130 to 50 km s 21 . The new sdata, in combination withHubble Space Telescope(HST) measurements of half-light radiiRe, indicate that these CNELGs are low-mass stellar systems (i.e.,M110 9 MJ),whiletheirunusuallylowmass-to-lightratios(typically ,0.2MJ/LJ)areconsistentwithbeing undergoing a major burst of star formation. SinceRe and sare roughly independent of the fading of the stellar population, theRe‐sdiagram is particularly useful for comparing the properties of these young galaxies to those of evolved stellar systems. Several physical processes that may modify the position of CNELGs in this diagram during their evolution, including dissipation, mergers, stripping, and winds, are discussed briefly. We conclude that the new data support a simple evolutionary scenario in which these low-mass, young galaxies will fade after the starburst, without major changes inRe or s, to become today’s spheroidal galaxies. Subject headings: cosmology: observations—galaxies: compact—galaxies: evolution—galaxies: formation— galaxies: fundamental parameters