Further insights into the structure of 30 Doradus from the Hubble space telescope instruments

New observations with the Hubble Space Telescope Wide Field Planetary Camera 2 (WFPC2), combined with prior archival data, provide nearly complete coverage of the inner 30 Doradus Nebula in both nebular lines and continuum at 0″.1 resolution. The developing windblown cavity surrounding the massive f...

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Autores principales: Walborn, Nolan Revere, Maíz Apellániz, Jesús, Barbá, Rodolfo Héctor
Formato: Articulo
Lenguaje:Inglés
Publicado: 2002
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/83519
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id I19-R120-10915-83519
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
Galaxies: starburst
H II regions
ISM: individual (30 Doradus)
Magellanic Clouds stars: early-type
Stars: formation
spellingShingle Ciencias Astronómicas
Galaxies: starburst
H II regions
ISM: individual (30 Doradus)
Magellanic Clouds stars: early-type
Stars: formation
Walborn, Nolan Revere
Maíz Apellániz, Jesús
Barbá, Rodolfo Héctor
Further insights into the structure of 30 Doradus from the Hubble space telescope instruments
topic_facet Ciencias Astronómicas
Galaxies: starburst
H II regions
ISM: individual (30 Doradus)
Magellanic Clouds stars: early-type
Stars: formation
description New observations with the Hubble Space Telescope Wide Field Planetary Camera 2 (WFPC2), combined with prior archival data, provide nearly complete coverage of the inner 30 Doradus Nebula in both nebular lines and continuum at 0″.1 resolution. The developing windblown cavity surrounding the massive first-generation, central cluster and its interface with the remanent molecular clouds, the site of second-generation, triggered star formation, are imaged in their entirety. Dithered Planetary Camera observations with 0″.03 resolution of Knots 1-3 reveal further structural details of the large dust pillars oriented toward the central cluster and the newborn, massive multiple systems of the second generation in those fields. The new data also provide the first WFPC2 coverage of the fields of two interesting, luminous infrared sources observed in our previous Near Infrared Camera and Multi-Object Spectrometer program; comparisons of the high-resolution optical and IR images are illuminating. In addition, we have obtained Space Telescope Imaging Spectrograph optical, long-slit observations of seven O-type multiple systems in the region, including those in Knots 1-3 and four representatives of the older generation. The spatially resolved spectrograms and classifications of the close pairs, with separations ranging from 0″.09 to 1″.18, are presented, as well as WFPC2 photometry of the individual components and the compact clusters of fainter stars associated with them. These new observations, and planned further analysis of them, offer significant new information about the intricate structure and evolution of the two-stage starburst in 30 Dor.
format Articulo
Articulo
author Walborn, Nolan Revere
Maíz Apellániz, Jesús
Barbá, Rodolfo Héctor
author_facet Walborn, Nolan Revere
Maíz Apellániz, Jesús
Barbá, Rodolfo Héctor
author_sort Walborn, Nolan Revere
title Further insights into the structure of 30 Doradus from the Hubble space telescope instruments
title_short Further insights into the structure of 30 Doradus from the Hubble space telescope instruments
title_full Further insights into the structure of 30 Doradus from the Hubble space telescope instruments
title_fullStr Further insights into the structure of 30 Doradus from the Hubble space telescope instruments
title_full_unstemmed Further insights into the structure of 30 Doradus from the Hubble space telescope instruments
title_sort further insights into the structure of 30 doradus from the hubble space telescope instruments
publishDate 2002
url http://sedici.unlp.edu.ar/handle/10915/83519
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AT barbarodolfohector furtherinsightsintothestructureof30doradusfromthehubblespacetelescopeinstruments
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