Toward Understanding the B[e] Phenomenon. II. New Galactic FS CMa Stars

Autores
Miroshnichenko, A. S.; Manset, N.; Kusakin, A.V.; Chentsov, E.L.; Klochkova, V. G.; Zharikov, S. V.; Gray, R. O.; Grankin, K. N.; Gandet, T. L.; Bjorkman, K. S.; Rudy, R. J.; Lynch, D. K.; Venturini, C. C.; Mazuk, S.; Puetter, R. C.; Perry, R. B.; Levato, Orlando Hugo; Grosso, Monica Gladys; Bernabei, S.; Polcaro, V. F.; Viotti, R. F.; Norci, L.; Kuratov, K. S.
Año de publicación
2007
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
FS CMa stars form a group of objects with the B[e] phenomenon that were previously known as unclassified B[e] stars or B[e] stars with warm dust (B[e]WD) until recently. They exhibit strong emission-line spectra and strong IR excesses, most likely due to recently formed circumstellar dust. These properties have been suggested to be due to ongoing or recent rapid mass exchange in binary systems with hot primaries and various types of secondaries. The first paper of this series reported an analysis of the available information about previously known Galactic objects with the B[e] phenomenon, the initial selection of the FS CMa group objects, and a qualitative explanation of their properties. This paper reports the results of our new search for more FS CMa objects in the IRAS Point Source Catalog. We present new photometric criteria for identifying FS CMa stars as well as the first results of our observations of nine new FS CMa group members. With this addition, the FS CMa group has now 40 members, becoming the largest among the dust-forming hot star groups. We also present nine objects with no evidence for the B[e] phenomenon, but with newly discovered spectral line emission and /or strong IR excesses.
Fil: Miroshnichenko, A. S.. The University Of North Carolina At Greensboro; Estados Unidos
Fil: Manset, N.. Canada France Hawaii Telescope; Estados Unidos
Fil: Kusakin, A.V.. Lomonosov Moscow State University; Rusia. Fesenkov Astrophysical Institute; Rusia
Fil: Chentsov, E.L.. Russian Academy Of Sciences; Rusia
Fil: Klochkova, V. G.. Russian Academy Of Sciences; Rusia
Fil: Zharikov, S. V.. Universidad Nacional Autónoma de México; México
Fil: Gray, R. O.. Appalachian State University (appstate);
Fil: Grankin, K. N.. Ulugh Beg Astronomical Institute Uzbekistan Academy Of Sciences; Uzbekistán
Fil: Gandet, T. L.. Lizard Hollow Observatory; Estados Unidos
Fil: Bjorkman, K. S.. University Of Toledo (utoledo); Estados Unidos
Fil: Rudy, R. J.. The Aerospace Corporation; Estados Unidos
Fil: Lynch, D. K.. The Aerospace Corporation; Estados Unidos
Fil: Venturini, C. C.. The Aerospace Corporation; Estados Unidos
Fil: Mazuk, S.. The Aerospace Corporation; Estados Unidos
Fil: Puetter, R. C.. University of California at San Diego; Estados Unidos
Fil: Perry, R. B.. National Aeronautics and Space Administration; Estados Unidos
Fil: Levato, Orlando Hugo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina
Fil: Grosso, Monica Gladys. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina
Fil: Bernabei, S.. Istituto Nazionale di Astrofisica; Italia
Fil: Polcaro, V. F.. Istituto Nazionale di Astrofisica; Italia
Fil: Viotti, R. F.. Istituto Nazionale di Astrofisica; Italia
Fil: Norci, L.. Dublin City University; Irlanda
Fil: Kuratov, K. S.. Fesenkov Astrophysical Institute; Kazajistán
Materia
CIRCUMSTELLAR MATTER
STARS: EARLY-TYPE
STARS: EMISSION-LINE, BE.
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:11336/214789
Acceder
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network_name_str CONICET Digital (CONICET)
spelling Toward Understanding the B[e] Phenomenon. II. New Galactic FS CMa StarsMiroshnichenko, A. S.Manset, N.Kusakin, A.V.Chentsov, E.L.Klochkova, V. G.Zharikov, S. V.Gray, R. O.Grankin, K. N.Gandet, T. L.Bjorkman, K. S.Rudy, R. J.Lynch, D. K.Venturini, C. C.Mazuk, S.Puetter, R. C.Perry, R. B.Levato, Orlando HugoGrosso, Monica GladysBernabei, S.Polcaro, V. F.Viotti, R. F.Norci, L.Kuratov, K. S.CIRCUMSTELLAR MATTERSTARS: EARLY-TYPESTARS: EMISSION-LINE, BE.https://purl.org/becyt/ford/1.7https://purl.org/becyt/ford/1FS CMa stars form a group of objects with the B[e] phenomenon that were previously known as unclassified B[e] stars or B[e] stars with warm dust (B[e]WD) until recently. They exhibit strong emission-line spectra and strong IR excesses, most likely due to recently formed circumstellar dust. These properties have been suggested to be due to ongoing or recent rapid mass exchange in binary systems with hot primaries and various types of secondaries. The first paper of this series reported an analysis of the available information about previously known Galactic objects with the B[e] phenomenon, the initial selection of the FS CMa group objects, and a qualitative explanation of their properties. This paper reports the results of our new search for more FS CMa objects in the IRAS Point Source Catalog. We present new photometric criteria for identifying FS CMa stars as well as the first results of our observations of nine new FS CMa group members. With this addition, the FS CMa group has now 40 members, becoming the largest among the dust-forming hot star groups. We also present nine objects with no evidence for the B[e] phenomenon, but with newly discovered spectral line emission and /or strong IR excesses.Fil: Miroshnichenko, A. S.. The University Of North Carolina At Greensboro; Estados UnidosFil: Manset, N.. Canada France Hawaii Telescope; Estados UnidosFil: Kusakin, A.V.. Lomonosov Moscow State University; Rusia. Fesenkov Astrophysical Institute; RusiaFil: Chentsov, E.L.. Russian Academy Of Sciences; RusiaFil: Klochkova, V. G.. Russian Academy Of Sciences; RusiaFil: Zharikov, S. V.. Universidad Nacional Autónoma de México; MéxicoFil: Gray, R. O.. Appalachian State University (appstate);Fil: Grankin, K. N.. Ulugh Beg Astronomical Institute Uzbekistan Academy Of Sciences; UzbekistánFil: Gandet, T. L.. Lizard Hollow Observatory; Estados UnidosFil: Bjorkman, K. S.. University Of Toledo (utoledo); Estados UnidosFil: Rudy, R. J.. The Aerospace Corporation; Estados UnidosFil: Lynch, D. K.. The Aerospace Corporation; Estados UnidosFil: Venturini, C. C.. The Aerospace Corporation; Estados UnidosFil: Mazuk, S.. The Aerospace Corporation; Estados UnidosFil: Puetter, R. C.. University of California at San Diego; Estados UnidosFil: Perry, R. B.. National Aeronautics and Space Administration; Estados UnidosFil: Levato, Orlando Hugo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; ArgentinaFil: Grosso, Monica Gladys. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; ArgentinaFil: Bernabei, S.. Istituto Nazionale di Astrofisica; ItaliaFil: Polcaro, V. F.. Istituto Nazionale di Astrofisica; ItaliaFil: Viotti, R. F.. Istituto Nazionale di Astrofisica; ItaliaFil: Norci, L.. Dublin City University; IrlandaFil: Kuratov, K. S.. Fesenkov Astrophysical Institute; KazajistánIOP Publishing2007-12info: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/11336/214789Miroshnichenko, A. S.; Manset, N.; Kusakin, A.V.; Chentsov, E.L.; Klochkova, V. G.; et al.; Toward Understanding the B[e] Phenomenon. II. New Galactic FS CMa Stars; IOP Publishing; Astrophysical Journal; 671; 1; 12-2007; 828-8410004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1086/523094info:eu-repo/semantics/altIdentifier/doi/10.1086/523094info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:37:03Zoai:ri.conicet.gov.ar:11336/214789instacron: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 09:37:03.501CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Toward Understanding the B[e] Phenomenon. II. New Galactic FS CMa Stars
title Toward Understanding the B[e] Phenomenon. II. New Galactic FS CMa Stars
spellingShingle Toward Understanding the B[e] Phenomenon. II. New Galactic FS CMa Stars
Miroshnichenko, A. S.
CIRCUMSTELLAR MATTER
STARS: EARLY-TYPE
STARS: EMISSION-LINE, BE.
title_short Toward Understanding the B[e] Phenomenon. II. New Galactic FS CMa Stars
title_full Toward Understanding the B[e] Phenomenon. II. New Galactic FS CMa Stars
title_fullStr Toward Understanding the B[e] Phenomenon. II. New Galactic FS CMa Stars
title_full_unstemmed Toward Understanding the B[e] Phenomenon. II. New Galactic FS CMa Stars
title_sort Toward Understanding the B[e] Phenomenon. II. New Galactic FS CMa Stars
dc.creator.none.fl_str_mv Miroshnichenko, A. S.
Manset, N.
Kusakin, A.V.
Chentsov, E.L.
Klochkova, V. G.
Zharikov, S. V.
Gray, R. O.
Grankin, K. N.
Gandet, T. L.
Bjorkman, K. S.
Rudy, R. J.
Lynch, D. K.
Venturini, C. C.
Mazuk, S.
Puetter, R. C.
Perry, R. B.
Levato, Orlando Hugo
Grosso, Monica Gladys
Bernabei, S.
Polcaro, V. F.
Viotti, R. F.
Norci, L.
Kuratov, K. S.
author Miroshnichenko, A. S.
author_facet Miroshnichenko, A. S.
Manset, N.
Kusakin, A.V.
Chentsov, E.L.
Klochkova, V. G.
Zharikov, S. V.
Gray, R. O.
Grankin, K. N.
Gandet, T. L.
Bjorkman, K. S.
Rudy, R. J.
Lynch, D. K.
Venturini, C. C.
Mazuk, S.
Puetter, R. C.
Perry, R. B.
Levato, Orlando Hugo
Grosso, Monica Gladys
Bernabei, S.
Polcaro, V. F.
Viotti, R. F.
Norci, L.
Kuratov, K. S.
author_role author
author2 Manset, N.
Kusakin, A.V.
Chentsov, E.L.
Klochkova, V. G.
Zharikov, S. V.
Gray, R. O.
Grankin, K. N.
Gandet, T. L.
Bjorkman, K. S.
Rudy, R. J.
Lynch, D. K.
Venturini, C. C.
Mazuk, S.
Puetter, R. C.
Perry, R. B.
Levato, Orlando Hugo
Grosso, Monica Gladys
Bernabei, S.
Polcaro, V. F.
Viotti, R. F.
Norci, L.
Kuratov, K. S.
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv CIRCUMSTELLAR MATTER
STARS: EARLY-TYPE
STARS: EMISSION-LINE, BE.
topic CIRCUMSTELLAR MATTER
STARS: EARLY-TYPE
STARS: EMISSION-LINE, BE.
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.7
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv FS CMa stars form a group of objects with the B[e] phenomenon that were previously known as unclassified B[e] stars or B[e] stars with warm dust (B[e]WD) until recently. They exhibit strong emission-line spectra and strong IR excesses, most likely due to recently formed circumstellar dust. These properties have been suggested to be due to ongoing or recent rapid mass exchange in binary systems with hot primaries and various types of secondaries. The first paper of this series reported an analysis of the available information about previously known Galactic objects with the B[e] phenomenon, the initial selection of the FS CMa group objects, and a qualitative explanation of their properties. This paper reports the results of our new search for more FS CMa objects in the IRAS Point Source Catalog. We present new photometric criteria for identifying FS CMa stars as well as the first results of our observations of nine new FS CMa group members. With this addition, the FS CMa group has now 40 members, becoming the largest among the dust-forming hot star groups. We also present nine objects with no evidence for the B[e] phenomenon, but with newly discovered spectral line emission and /or strong IR excesses.
Fil: Miroshnichenko, A. S.. The University Of North Carolina At Greensboro; Estados Unidos
Fil: Manset, N.. Canada France Hawaii Telescope; Estados Unidos
Fil: Kusakin, A.V.. Lomonosov Moscow State University; Rusia. Fesenkov Astrophysical Institute; Rusia
Fil: Chentsov, E.L.. Russian Academy Of Sciences; Rusia
Fil: Klochkova, V. G.. Russian Academy Of Sciences; Rusia
Fil: Zharikov, S. V.. Universidad Nacional Autónoma de México; México
Fil: Gray, R. O.. Appalachian State University (appstate);
Fil: Grankin, K. N.. Ulugh Beg Astronomical Institute Uzbekistan Academy Of Sciences; Uzbekistán
Fil: Gandet, T. L.. Lizard Hollow Observatory; Estados Unidos
Fil: Bjorkman, K. S.. University Of Toledo (utoledo); Estados Unidos
Fil: Rudy, R. J.. The Aerospace Corporation; Estados Unidos
Fil: Lynch, D. K.. The Aerospace Corporation; Estados Unidos
Fil: Venturini, C. C.. The Aerospace Corporation; Estados Unidos
Fil: Mazuk, S.. The Aerospace Corporation; Estados Unidos
Fil: Puetter, R. C.. University of California at San Diego; Estados Unidos
Fil: Perry, R. B.. National Aeronautics and Space Administration; Estados Unidos
Fil: Levato, Orlando Hugo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina
Fil: Grosso, Monica Gladys. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina
Fil: Bernabei, S.. Istituto Nazionale di Astrofisica; Italia
Fil: Polcaro, V. F.. Istituto Nazionale di Astrofisica; Italia
Fil: Viotti, R. F.. Istituto Nazionale di Astrofisica; Italia
Fil: Norci, L.. Dublin City University; Irlanda
Fil: Kuratov, K. S.. Fesenkov Astrophysical Institute; Kazajistán
description FS CMa stars form a group of objects with the B[e] phenomenon that were previously known as unclassified B[e] stars or B[e] stars with warm dust (B[e]WD) until recently. They exhibit strong emission-line spectra and strong IR excesses, most likely due to recently formed circumstellar dust. These properties have been suggested to be due to ongoing or recent rapid mass exchange in binary systems with hot primaries and various types of secondaries. The first paper of this series reported an analysis of the available information about previously known Galactic objects with the B[e] phenomenon, the initial selection of the FS CMa group objects, and a qualitative explanation of their properties. This paper reports the results of our new search for more FS CMa objects in the IRAS Point Source Catalog. We present new photometric criteria for identifying FS CMa stars as well as the first results of our observations of nine new FS CMa group members. With this addition, the FS CMa group has now 40 members, becoming the largest among the dust-forming hot star groups. We also present nine objects with no evidence for the B[e] phenomenon, but with newly discovered spectral line emission and /or strong IR excesses.
publishDate 2007
dc.date.none.fl_str_mv 2007-12
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/11336/214789
Miroshnichenko, A. S.; Manset, N.; Kusakin, A.V.; Chentsov, E.L.; Klochkova, V. G.; et al.; Toward Understanding the B[e] Phenomenon. II. New Galactic FS CMa Stars; IOP Publishing; Astrophysical Journal; 671; 1; 12-2007; 828-841
0004-637X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/214789
identifier_str_mv Miroshnichenko, A. S.; Manset, N.; Kusakin, A.V.; Chentsov, E.L.; Klochkova, V. G.; et al.; Toward Understanding the B[e] Phenomenon. II. New Galactic FS CMa Stars; IOP Publishing; Astrophysical Journal; 671; 1; 12-2007; 828-841
0004-637X
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1086/523094
info:eu-repo/semantics/altIdentifier/doi/10.1086/523094
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 IOP Publishing
publisher.none.fl_str_mv IOP Publishing
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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