VLA radio continuum and IRAS observations of the ring nebulae around WR 101 and WR 113

We report radio continuum observations at 1465 MHz obtained with the Very Large Array (VLA) in the DnC configuration toward the ring nebulae associated with the stars WR 101 and WR 113, with resolutions of ∼38″ and 30″, respectively. IRAS images of the nebulae with resolutions of about 2′ (90 M⊙, 40...

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Detalles Bibliográficos
Autores principales: Cappa, Cristina Elisabet, Goss, W. M., Pineault, Serge
Formato: Articulo
Lenguaje:Inglés
Publicado: 2002
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/84623
Aporte de:
id I19-R120-10915-84623
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
ISM: bubbles
ISM: individual (Anon. WR 101, Anon WR 113)
Stars: individual (WR 101, WR 113)
Stars: Wolf-Rayet
spellingShingle Ciencias Astronómicas
ISM: bubbles
ISM: individual (Anon. WR 101, Anon WR 113)
Stars: individual (WR 101, WR 113)
Stars: Wolf-Rayet
Cappa, Cristina Elisabet
Goss, W. M.
Pineault, Serge
VLA radio continuum and IRAS observations of the ring nebulae around WR 101 and WR 113
topic_facet Ciencias Astronómicas
ISM: bubbles
ISM: individual (Anon. WR 101, Anon WR 113)
Stars: individual (WR 101, WR 113)
Stars: Wolf-Rayet
description We report radio continuum observations at 1465 MHz obtained with the Very Large Array (VLA) in the DnC configuration toward the ring nebulae associated with the stars WR 101 and WR 113, with resolutions of ∼38″ and 30″, respectively. IRAS images of the nebulae with resolutions of about 2′ (90 M⊙, 40 cm<SUP>-3</SUP>) are also analyzed. A remarkable resemblance among the optical, infrared, and radio images of these ring nebulae is observed. The VLA data indicate that Anon. WR 101 is thermal in nature. An ionized mass of ≈230 ± 40 M⊙ and electron densities in the range ≈40-55 cm<SUP>-3</SUP> were estimated for Anon. WR 101. The derived ionized masses and electron densities in the inner and outer shells of the nebula related to WR 113 are ≈20 ± 10 M⊙, 180-500 cm<SUP>-3</SUP> and ≈90 M⊙ 40 cm<SUP>-3</SUP>, respectively. Based on infrared data at 60 and 100 μm, the derived masses and temperatures for the dust component in the ring nebula around WR 101 are 0.3-1 M⊙ and ≈40 K. The associated masses suggest that the ring nebula related to WR 101 and the outer arc associated with WR 113 consist of swept-up interstellar matter, while the relatively low ionized mass associated with the inner shell of the nebula around WR 113 may contain a nonnegligible contribution of expelled ejecta material. The derived electron densities for the nebula around WR 101 and the inner shell around WR 113 are comparable to electron densities for other W-R ring nebulae. Low filling factors are inferred for both nebulae. The nebulae probably originated during the current W-R phase of the stars.
format Articulo
Articulo
author Cappa, Cristina Elisabet
Goss, W. M.
Pineault, Serge
author_facet Cappa, Cristina Elisabet
Goss, W. M.
Pineault, Serge
author_sort Cappa, Cristina Elisabet
title VLA radio continuum and IRAS observations of the ring nebulae around WR 101 and WR 113
title_short VLA radio continuum and IRAS observations of the ring nebulae around WR 101 and WR 113
title_full VLA radio continuum and IRAS observations of the ring nebulae around WR 101 and WR 113
title_fullStr VLA radio continuum and IRAS observations of the ring nebulae around WR 101 and WR 113
title_full_unstemmed VLA radio continuum and IRAS observations of the ring nebulae around WR 101 and WR 113
title_sort vla radio continuum and iras observations of the ring nebulae around wr 101 and wr 113
publishDate 2002
url http://sedici.unlp.edu.ar/handle/10915/84623
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AT gosswm vlaradiocontinuumandirasobservationsoftheringnebulaearoundwr101andwr113
AT pineaultserge vlaradiocontinuumandirasobservationsoftheringnebulaearoundwr101andwr113
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