3,657 research outputs found
CO observations and investigation of triggered star formation towards N10 infrared bubble and surroundings
We studied the environment of the dust bubble N10 in molecular emission.
Infrared bubbles, first detected by the GLIMPSE survey at 8.0 m, are ideal
regions to investigate the effect of the expansion of the HII region on its
surroundings eventual triggered star formation at its borders. In this work, we
present a multi-wavelength study of N10. This bubble is especially interesting
as infrared studies of the young stellar content suggest a scenario of ongoing
star formation, possibly triggered, on the edge of the HII region. We carried
out observations of CO(1-0) and CO(1-0) emission at PMO 13.7-m
towards N10. We also analyzed the IR and sub-mm emission on this region and
compare those different tracers to obtain a detailed view of the interaction
between the expanding HII region and the molecular gas. We also estimated the
parameters of the denser cold dust condensation and of the ionized gas inside
the shell. Bright CO emission was detected and two molecular clumps were
identified, from which we have derived physical parameters. We also estimate
the parameters for the densest cold dust condensation and for the ionized gas
inside the shell. The comparison between the dynamical age of this region and
the fragmentation time scale favors the "Radiation-Driven Implosion" mechanism
of star formation. N10 reveals to be specially interesting case with gas
structures in a narrow frontier between HII region and surrounding molecular
material, and with a range of ages of YSOs situated in region indicating
triggered star formation.Comment: Version 2 - Submmited to ApJ (under review
Capacidade de combinação e heterose em hĂbridos intervarietais de milho (Zea mays L.) adaptadas as condições de cerrados.
Depressão por endogamia de diversas populações de milho (Zea mays L.) introduzidas no Brasil.
Antifouling activity as a function of population variation in Sargassum vulgare from the littoral of Rio de Janeiro (Brazil)
Adaptabilidade e estabilidade de produção de grĂŁos de genĂłtipos de milho melhorados para o EspĂrito Santo.
General and specific combinig ability for yield in a diallel cross among 18 maize populations (Zea mays L.).
A study was carried out no diallel crosses among 18 maize populations. An analysis was conducted on ear weight data using Grigging's Method 2, Model I to determine general and specific combinig ability effects. General combining ability (GCA) was found to be significant but specific combinig ability (SCA) was not. Both location x GCA and location x SCA interactions were found to be significant. The results showed that populations CMS 06 and CMS 05 have the highest GCA effects. The cross (CMS 07 x CMS 10) gave the highest SCA effects
Capacidade de combinação e heterose em hĂbridos intervarietais de milho adaptados a solos ácidos.
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