other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
2002MNRAS.337.1309S - Mon. Not. R. Astron. Soc., 337, 1309-1328 (2002/December-3)
Realistic ionizing fluxes for young stellar populations from 0.05 to 2 Z☉.
SMITH L.J., NORRIS R.P.F. and CROWTHER P.A.
Abstract (from CDS):
We incorporate the new models into the evolutionary synthesis code starburst99 and compare the ionizing outputs for an instantaneous burst and continuous star formation with the work of Schaerer & Vacca (SV98), and Leitherer et al. The changes in the output ionizing fluxes as a function of age are dramatic. We find that, in contrast to previous studies, nebular Heiiλ4686 will be at, or just below, the detection limit in low metallicity starbursts during the W-R phase. The new models have lower fluxes in the Hei continuum for Z ≥ 0.4 Z☉and ages ≤7 Myr because of the increased line blanketing.
We test the accuracy of the new model atmosphere grid by constructing photoionization models for simple HII regions, and assessing the impact of the new ionizing fluxes on important nebular diagnostic line ratios. For the case of an HII region where the ionizing flux is given by the WM-basic dwarf O star grid, we show that Heiλ5786/Hβ decreases between 1 and 2 Z☉in a similar manner to observations. We find that this decline is caused by the increased effect of line blanketing above solar metallicity. We therefore suggest that a lowering of the upper mass limit at high abundances is not required to explain the diminishing strength of Heiλ5786/Hβ, as has been suggested in the past. For an HII region where the ionizing flux is provided by an instantaneous burst of total mass 106 M☉, we plot the softness parameter η' against the abundance indicator R23for ages of 1-5 Myr. The new models are coincident with the observational data of Bresolin et al., particularly during the W-R phase, unlike the previous models of SV98 which generally over-predict the hardness of the ionizing radiation.
The new model grid and updated starburst99 code can be downloaded from http://www.star.ucl.ac.uk/starburst.
Abstract Copyright: RAS
Journal keyword(s): stars: atmospheres - stars: mass-loss - stars: Wolf-Rayet - HII regions - galaxies: starburst - galaxies: stellar content
Simbad objects: 5
To bookmark this query, right click on this link: simbad:2002MNRAS.337.1309S and select 'bookmark this link' or equivalent in the popup menu