Imagem composta do anel de Einstein da SDP.81 e da galáxia reconstruída
A Campanha de Linha de Base Longa do ALMA produziu uma imagem muito detalhada de uma galáxia distante afectada por lente gravitacional, que revela regiões de formação estelar — algo que nunca tinha sido observado antes com este nível de detalhe numa galáxia tão remota. As novas observações são muito mais detalhadas do que as obtidas anteriormente para esta galáxia, incluindo as do Telescópio Espacial Hubble da NASA/ESA e revelam nodos de formação estelar na galáxia equivalentes a versões gigantes da Nebulosa de Orion.
O painel da esquerda revela a galáxia que se encontra em primeiro plano e que atua como lente gravitacional (observada pelo Hubble), enquanto que a galáxia distante que está a ser afectada pela lente, a SDP.81, e que forma um anel de Einstein quase perfeito, praticamente não se vê.
A imagem do meio mostra a imagem muito nítida do ALMA com o anel de Einstein, sendo que a galáxia que atua como lente é invisível para o ALMA. A imagem da galáxia distante (à direita), reconstruída com o auxílio de modelos sofisticados de lente gravitacional, revela estruturas detalhadas no interior do anel, que nunca tinham sido observadas anteriormente: várias nuvens de poeira no seio da galáxia, que se pensa serem nuvens moleculares gigantes e frias, o local de nascimento de estrelas e planetas.
ALMA (NRAO/ESO/NAOJ)/Y. Tamura (The University of Tokyo)/Mark Swinbank (Durham University)
Sobre a imagem
Id: | eso1522a |
Língua: | pt |
Tipo: | Montagem |
Data de divulgação: | 8 de Junho de 2015 às 20:00 |
Notícias relacionadas: | eso1522 |
Tamanho: | 2537 x 928 px |
Sobre o objeto
Nome: | Einstein Ring, H-ATLAS J090311.6+003906, SDP 81 |
Tipo: | Early Universe : Galaxy : Type : Gravitationally Lensed Early Universe : Cosmology : Phenomenon : Lensing |
Distância: | z=3.04 (desvio para o vermelho) |
Formatos de imagens
Cores e filtros
Banda | Telescópio |
---|---|
Milímetro | Atacama Large Millimeter/submillimeter Array |
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