The infrared Hourglass cluster in M8

Autores
Arias, Julia Ines; Barba, Rodolfo Hector; Maíz Apellániz, J.; Morrell, Nidia Irene; Rubio, M.
Año de publicación
2006
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
A detailed study of the Hourglass nebula in the M8 star-forming region is presented. The study is mainly based on recent subarcsec-resolution JHK s images taken at Las Campanas Observatory and complemented with archival Hubble Space Telescope (HST) images and long-slit spectroscopy retrieved from the European Southern Observatory Archive Facility. Using the new numerical code chorizos, we estimate the distance to the earliest stars in the region to be 1.25 kpc. Infrared photometry of all the sources detected in the field is given. From analysis of the JHKs colour-colour diagrams, we find that an important fraction of these sources exhibit significant infrared excess. These objects are candidates to be low- and intermediate-mass pre-main-sequence stars. Based on HST observations, the spatial distribution of gas, dust and stars in the region is analysed. A morphological analysis of these images also reveals a rich variety of structures related to star formation (proplyds, jets, bow shocks), similar to those observed in M16 and M42, along with the detection of the first four Herbig-Haro objects in the region. Furthermore, a long-slit spectrum obtained with the New Technology Telescope confirms the identification of one of them (HH 870) in the core of the Hourglass nebula, providing the first direct evidence of active star formation by accretion in M8.
Fil: Arias, Julia Ines. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Barba, Rodolfo Hector. Universidad de La Serena; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Maíz Apellániz, J.. Space Telescope Science Institute; Estados Unidos
Fil: Morrell, Nidia Irene. Las Campanas Observatory; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Rubio, M.. Universidad de Chile; Chile
Materia
H II REGIONS
ISM: HERBIG-HARO OBJECTS
ISM: JETS AND OUTFLOWS
STARS: FORMATION
STARS: PRE-MAIN-SEQUENCE
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/38213
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/38213
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling The infrared Hourglass cluster in M8Arias, Julia InesBarba, Rodolfo HectorMaíz Apellániz, J.Morrell, Nidia IreneRubio, M.H II REGIONSISM: HERBIG-HARO OBJECTSISM: JETS AND OUTFLOWSSTARS: FORMATIONSTARS: PRE-MAIN-SEQUENCEhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1A detailed study of the Hourglass nebula in the M8 star-forming region is presented. The study is mainly based on recent subarcsec-resolution JHK s images taken at Las Campanas Observatory and complemented with archival Hubble Space Telescope (HST) images and long-slit spectroscopy retrieved from the European Southern Observatory Archive Facility. Using the new numerical code chorizos, we estimate the distance to the earliest stars in the region to be 1.25 kpc. Infrared photometry of all the sources detected in the field is given. From analysis of the JHKs colour-colour diagrams, we find that an important fraction of these sources exhibit significant infrared excess. These objects are candidates to be low- and intermediate-mass pre-main-sequence stars. Based on HST observations, the spatial distribution of gas, dust and stars in the region is analysed. A morphological analysis of these images also reveals a rich variety of structures related to star formation (proplyds, jets, bow shocks), similar to those observed in M16 and M42, along with the detection of the first four Herbig-Haro objects in the region. Furthermore, a long-slit spectrum obtained with the New Technology Telescope confirms the identification of one of them (HH 870) in the core of the Hourglass nebula, providing the first direct evidence of active star formation by accretion in M8.Fil: Arias, Julia Ines. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Barba, Rodolfo Hector. Universidad de La Serena; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Maíz Apellániz, J.. Space Telescope Science Institute; Estados UnidosFil: Morrell, Nidia Irene. Las Campanas Observatory; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Rubio, M.. Universidad de Chile; ChileOxford University Press2006-03info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/38213Arias, Julia Ines; Barba, Rodolfo Hector; Maíz Apellániz, J.; Morrell, Nidia Irene; Rubio, M.; The infrared Hourglass cluster in M8; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 366; 3; 3-2006; 739-7570035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2005.09829.xinfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/366/3/739/992534info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:07:53Zoai:ri.conicet.gov.ar:11336/38213instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:07:54.078CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv The infrared Hourglass cluster in M8
title The infrared Hourglass cluster in M8
spellingShingle The infrared Hourglass cluster in M8
Arias, Julia Ines
H II REGIONS
ISM: HERBIG-HARO OBJECTS
ISM: JETS AND OUTFLOWS
STARS: FORMATION
STARS: PRE-MAIN-SEQUENCE
title_short The infrared Hourglass cluster in M8
title_full The infrared Hourglass cluster in M8
title_fullStr The infrared Hourglass cluster in M8
title_full_unstemmed The infrared Hourglass cluster in M8
title_sort The infrared Hourglass cluster in M8
dc.creator.none.fl_str_mv Arias, Julia Ines
Barba, Rodolfo Hector
Maíz Apellániz, J.
Morrell, Nidia Irene
Rubio, M.
author Arias, Julia Ines
author_facet Arias, Julia Ines
Barba, Rodolfo Hector
Maíz Apellániz, J.
Morrell, Nidia Irene
Rubio, M.
author_role author
author2 Barba, Rodolfo Hector
Maíz Apellániz, J.
Morrell, Nidia Irene
Rubio, M.
author2_role author
author
author
author
dc.subject.none.fl_str_mv H II REGIONS
ISM: HERBIG-HARO OBJECTS
ISM: JETS AND OUTFLOWS
STARS: FORMATION
STARS: PRE-MAIN-SEQUENCE
topic H II REGIONS
ISM: HERBIG-HARO OBJECTS
ISM: JETS AND OUTFLOWS
STARS: FORMATION
STARS: PRE-MAIN-SEQUENCE
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv A detailed study of the Hourglass nebula in the M8 star-forming region is presented. The study is mainly based on recent subarcsec-resolution JHK s images taken at Las Campanas Observatory and complemented with archival Hubble Space Telescope (HST) images and long-slit spectroscopy retrieved from the European Southern Observatory Archive Facility. Using the new numerical code chorizos, we estimate the distance to the earliest stars in the region to be 1.25 kpc. Infrared photometry of all the sources detected in the field is given. From analysis of the JHKs colour-colour diagrams, we find that an important fraction of these sources exhibit significant infrared excess. These objects are candidates to be low- and intermediate-mass pre-main-sequence stars. Based on HST observations, the spatial distribution of gas, dust and stars in the region is analysed. A morphological analysis of these images also reveals a rich variety of structures related to star formation (proplyds, jets, bow shocks), similar to those observed in M16 and M42, along with the detection of the first four Herbig-Haro objects in the region. Furthermore, a long-slit spectrum obtained with the New Technology Telescope confirms the identification of one of them (HH 870) in the core of the Hourglass nebula, providing the first direct evidence of active star formation by accretion in M8.
Fil: Arias, Julia Ines. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Barba, Rodolfo Hector. Universidad de La Serena; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Maíz Apellániz, J.. Space Telescope Science Institute; Estados Unidos
Fil: Morrell, Nidia Irene. Las Campanas Observatory; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Rubio, M.. Universidad de Chile; Chile
description A detailed study of the Hourglass nebula in the M8 star-forming region is presented. The study is mainly based on recent subarcsec-resolution JHK s images taken at Las Campanas Observatory and complemented with archival Hubble Space Telescope (HST) images and long-slit spectroscopy retrieved from the European Southern Observatory Archive Facility. Using the new numerical code chorizos, we estimate the distance to the earliest stars in the region to be 1.25 kpc. Infrared photometry of all the sources detected in the field is given. From analysis of the JHKs colour-colour diagrams, we find that an important fraction of these sources exhibit significant infrared excess. These objects are candidates to be low- and intermediate-mass pre-main-sequence stars. Based on HST observations, the spatial distribution of gas, dust and stars in the region is analysed. A morphological analysis of these images also reveals a rich variety of structures related to star formation (proplyds, jets, bow shocks), similar to those observed in M16 and M42, along with the detection of the first four Herbig-Haro objects in the region. Furthermore, a long-slit spectrum obtained with the New Technology Telescope confirms the identification of one of them (HH 870) in the core of the Hourglass nebula, providing the first direct evidence of active star formation by accretion in M8.
publishDate 2006
dc.date.none.fl_str_mv 2006-03
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/38213
Arias, Julia Ines; Barba, Rodolfo Hector; Maíz Apellániz, J.; Morrell, Nidia Irene; Rubio, M.; The infrared Hourglass cluster in M8; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 366; 3; 3-2006; 739-757
0035-8711
CONICET Digital
CONICET
url http://hdl.handle.net/11336/38213
identifier_str_mv Arias, Julia Ines; Barba, Rodolfo Hector; Maíz Apellániz, J.; Morrell, Nidia Irene; Rubio, M.; The infrared Hourglass cluster in M8; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 366; 3; 3-2006; 739-757
0035-8711
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2005.09829.x
info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/366/3/739/992534
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
application/pdf
dc.publisher.none.fl_str_mv Oxford University Press
publisher.none.fl_str_mv Oxford University Press
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 13.070432

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