VVV study of the young Milky Way star clusters: Mercer 35, 69 and 70

Radostin Kurtev, Jura Borissova, Charles Bonatto, Francisco Peñaloza, Valentin Ivanov, Étienne Artigau, Stuart Folkes, Douglas Geisler, Dante Minniti, Philip Lucas, Stuart Sale

Resultado de la investigación: Conference contribution

Resumen

Young massive clusters are usually deeply embedded in dust and gas. They represent excellent astrophysical laboratories for revealing the enigma of star formation processes and the early stages of stellar evolution. Wide-field infrared surveys are a modern tool for studying hidden clusters. "Vista variables in Vía Láctea - VVV" (Minniti et al. New Astron. 15:433, 2010) is an ESO/Chile/VISTA public deep near-IR survey, covering the Galactic Bulge and Southern Galactic disk. This is the next step of our systematic study of the cluster content of the inner Milky Way. Here we present our first analysis of the young hidden clusters Mercer 35, 69 and 70. It is based on VVV and SOFI/NTT JHKS photometry and follow-up NIR spectroscopy. All of the investigated clusters are young (t≤10 Myr). The basic cluster parameters are obtained from photometry. The follow-up spectroscopy of probable cluster members shows that the brightest star in Mercer 35 presents characteristics of a red supergiant!

Idioma originalEnglish
Título de la publicación alojadaStar Clusters in the Era of Large Surveys - Proceedings of Symposium 5 of JENAM 2010
EditorialKluwer Academic Publishers
Páginas109-111
Número de páginas3
ISBN (versión impresa)9783642221125
DOI
EstadoPublished - 2012
Evento5th JENAM Symposium: Star Clusters in the Era of Large Surveys, JENAM 2010 - Lisbon, Portugal
Duración: 9 sep 201010 sep 2010

Other

Other5th JENAM Symposium: Star Clusters in the Era of Large Surveys, JENAM 2010
PaísPortugal
CiudadLisbon
Período9/09/1010/09/10

Huella dactilar

star clusters
photometry
galactic bulge
Chile
stellar evolution
European Southern Observatory
spectroscopy
star formation
astrophysics
coverings
dust
stars
gases

ASJC Scopus subject areas

  • Astronomy and Astrophysics

Citar esto

Kurtev, R., Borissova, J., Bonatto, C., Peñaloza, F., Ivanov, V., Artigau, É., ... Sale, S. (2012). VVV study of the young Milky Way star clusters: Mercer 35, 69 and 70. En Star Clusters in the Era of Large Surveys - Proceedings of Symposium 5 of JENAM 2010 (pp. 109-111). Kluwer Academic Publishers. https://doi.org/10.1007/978-3-642-22113-2-16
Kurtev, Radostin ; Borissova, Jura ; Bonatto, Charles ; Peñaloza, Francisco ; Ivanov, Valentin ; Artigau, Étienne ; Folkes, Stuart ; Geisler, Douglas ; Minniti, Dante ; Lucas, Philip ; Sale, Stuart. / VVV study of the young Milky Way star clusters : Mercer 35, 69 and 70. Star Clusters in the Era of Large Surveys - Proceedings of Symposium 5 of JENAM 2010. Kluwer Academic Publishers, 2012. pp. 109-111
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title = "VVV study of the young Milky Way star clusters: Mercer 35, 69 and 70",
abstract = "Young massive clusters are usually deeply embedded in dust and gas. They represent excellent astrophysical laboratories for revealing the enigma of star formation processes and the early stages of stellar evolution. Wide-field infrared surveys are a modern tool for studying hidden clusters. {"}Vista variables in V{\'i}a L{\'a}ctea - VVV{"} (Minniti et al. New Astron. 15:433, 2010) is an ESO/Chile/VISTA public deep near-IR survey, covering the Galactic Bulge and Southern Galactic disk. This is the next step of our systematic study of the cluster content of the inner Milky Way. Here we present our first analysis of the young hidden clusters Mercer 35, 69 and 70. It is based on VVV and SOFI/NTT JHKS photometry and follow-up NIR spectroscopy. All of the investigated clusters are young (t≤10 Myr). The basic cluster parameters are obtained from photometry. The follow-up spectroscopy of probable cluster members shows that the brightest star in Mercer 35 presents characteristics of a red supergiant!",
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Kurtev, R, Borissova, J, Bonatto, C, Peñaloza, F, Ivanov, V, Artigau, É, Folkes, S, Geisler, D, Minniti, D, Lucas, P & Sale, S 2012, VVV study of the young Milky Way star clusters: Mercer 35, 69 and 70. En Star Clusters in the Era of Large Surveys - Proceedings of Symposium 5 of JENAM 2010. Kluwer Academic Publishers, pp. 109-111, 5th JENAM Symposium: Star Clusters in the Era of Large Surveys, JENAM 2010, Lisbon, Portugal, 9/09/10. https://doi.org/10.1007/978-3-642-22113-2-16

VVV study of the young Milky Way star clusters : Mercer 35, 69 and 70. / Kurtev, Radostin; Borissova, Jura; Bonatto, Charles; Peñaloza, Francisco; Ivanov, Valentin; Artigau, Étienne; Folkes, Stuart; Geisler, Douglas; Minniti, Dante; Lucas, Philip; Sale, Stuart.

Star Clusters in the Era of Large Surveys - Proceedings of Symposium 5 of JENAM 2010. Kluwer Academic Publishers, 2012. p. 109-111.

Resultado de la investigación: Conference contribution

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AU - Kurtev, Radostin

AU - Borissova, Jura

AU - Bonatto, Charles

AU - Peñaloza, Francisco

AU - Ivanov, Valentin

AU - Artigau, Étienne

AU - Folkes, Stuart

AU - Geisler, Douglas

AU - Minniti, Dante

AU - Lucas, Philip

AU - Sale, Stuart

PY - 2012

Y1 - 2012

N2 - Young massive clusters are usually deeply embedded in dust and gas. They represent excellent astrophysical laboratories for revealing the enigma of star formation processes and the early stages of stellar evolution. Wide-field infrared surveys are a modern tool for studying hidden clusters. "Vista variables in Vía Láctea - VVV" (Minniti et al. New Astron. 15:433, 2010) is an ESO/Chile/VISTA public deep near-IR survey, covering the Galactic Bulge and Southern Galactic disk. This is the next step of our systematic study of the cluster content of the inner Milky Way. Here we present our first analysis of the young hidden clusters Mercer 35, 69 and 70. It is based on VVV and SOFI/NTT JHKS photometry and follow-up NIR spectroscopy. All of the investigated clusters are young (t≤10 Myr). The basic cluster parameters are obtained from photometry. The follow-up spectroscopy of probable cluster members shows that the brightest star in Mercer 35 presents characteristics of a red supergiant!

AB - Young massive clusters are usually deeply embedded in dust and gas. They represent excellent astrophysical laboratories for revealing the enigma of star formation processes and the early stages of stellar evolution. Wide-field infrared surveys are a modern tool for studying hidden clusters. "Vista variables in Vía Láctea - VVV" (Minniti et al. New Astron. 15:433, 2010) is an ESO/Chile/VISTA public deep near-IR survey, covering the Galactic Bulge and Southern Galactic disk. This is the next step of our systematic study of the cluster content of the inner Milky Way. Here we present our first analysis of the young hidden clusters Mercer 35, 69 and 70. It is based on VVV and SOFI/NTT JHKS photometry and follow-up NIR spectroscopy. All of the investigated clusters are young (t≤10 Myr). The basic cluster parameters are obtained from photometry. The follow-up spectroscopy of probable cluster members shows that the brightest star in Mercer 35 presents characteristics of a red supergiant!

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SN - 9783642221125

SP - 109

EP - 111

BT - Star Clusters in the Era of Large Surveys - Proceedings of Symposium 5 of JENAM 2010

PB - Kluwer Academic Publishers

ER -

Kurtev R, Borissova J, Bonatto C, Peñaloza F, Ivanov V, Artigau É y otros. VVV study of the young Milky Way star clusters: Mercer 35, 69 and 70. En Star Clusters in the Era of Large Surveys - Proceedings of Symposium 5 of JENAM 2010. Kluwer Academic Publishers. 2012. p. 109-111 https://doi.org/10.1007/978-3-642-22113-2-16