SciELO - Scientific Electronic Library Online

 
vol.54 número1In situ orbit extraction from live, high precision collisions simulations of systems formed by cold collapseHigh astrometric precision in the calculation of the coordinates of orbiters in the GEO ring índice de autoresíndice de assuntospesquisa de artigos
Home Pagelista alfabética de periódicos  

Serviços Personalizados

Journal

Artigo

Indicadores

Links relacionados

  • Não possue artigos similaresSimilares em SciELO

Compartilhar


Revista mexicana de astronomía y astrofísica

versão impressa ISSN 0185-1101

Resumo

RAGA, A. C. et al. The time-dependent wavelet spectrum of HH 1 and 2. Rev. mex. astron. astrofis [online]. 2018, vol.54, n.1. ISSN 0185-1101.

We have calculated the wavelet spectra of four epochs (spanning ≈ 20 yr) of Hα and [S II] HST images of HH 1 and 2. From these spectra we calculated the distribution functions of the (angular) radii of the emission structures. We found that the size distributions have maxima (corresponding to the characteristic sizes of the observed structures) with radii that are logarithmically spaced with factors of ≈ 2 → 3 between the successive peaks. The positions of these peaks generally showed small shifts towards larger sizes as a function of time. This result indicates that the structures of HH 1 and 2 have a general expansion (seen at all scales), and/or are the result of a sequence of merging events resulting in the formation of knots with larger characteristic sizes.

Palavras-chave : Herbig-Haro objects; ISM: individual objects (HH1/2); ISM: jets and outflows; ISM: kinematics and dynamics; shock waves; stars: winds; outflows.

        · resumo em Espanhol     · texto em Inglês     · Inglês ( pdf )