Tracing the structure of the Perseus arm with IPHAS

Roberto Raddi; J.E. Drew; S.E. Sale; D.T.H. Steeghs

doi:10.1007/978-3-642-22113-2_48

Tracing the structure of the Perseus arm with IPHAS

Roberto Raddi, J.E. Drew, S.E. Sale, D.T.H. Steeghs

Centre for Astrophysics Research (CAR)

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

Research aiming to describe the spiral structure of the Milky Way disc has to confront both difficulties in obtaining distances and the high interstellar extinction found in the Galactic plane. We present a study of a section of the Perseus Arm, between Galactic longitudes. (120°, 140°) and Galactic latitudes .(-1°+4°), including a number of young clusters. Determination of physical parameters of young stellar objects (YSO) and mapping of the A-star surface density are used to analyse evidence of young structures (typically 10-100 Myrs old) defined in space

Original language	English
Title of host publication	Star Clusters in the Era of Large Surveys
Subtitle of host publication	Proceedings of Symposium 5 of JENAM 2010
Editors	A. Moitinho, J. Alves
Publisher	Springer Nature Link
Pages	259-260
Number of pages	2
ISBN (Electronic)	978-3-642-2213-2
ISBN (Print)	978-364222112-5
DOIs	https://doi.org/10.1007/978-3-642-22113-2_48
Publication status	Published - 2012
Event	5th JENAM Symposium - Lisbon, Portugal Duration: 9 Sept 2010 → 10 Sept 2010

Publication series

Name	Astrophysics and Space Science Proceedings

Conference

Conference	5th JENAM Symposium
Country/Territory	Portugal
Period	9/09/10 → 10/09/10

Access to Document

10.1007/978-3-642-22113-2_48

Cite this

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title = "Tracing the structure of the Perseus arm with IPHAS",

abstract = "Research aiming to describe the spiral structure of the Milky Way disc has to confront both difficulties in obtaining distances and the high interstellar extinction found in the Galactic plane. We present a study of a section of the Perseus Arm, between Galactic longitudes. (120°, 140°) and Galactic latitudes .(-1°+4°), including a number of young clusters. Determination of physical parameters of young stellar objects (YSO) and mapping of the A-star surface density are used to analyse evidence of young structures (typically 10-100 Myrs old) defined in space",

author = "Roberto Raddi and J.E. Drew and S.E. Sale and D.T.H. Steeghs",

year = "2012",

doi = "10.1007/978-3-642-22113-2_48",

language = "English",

isbn = "978-364222112-5",

series = "Astrophysics and Space Science Proceedings",

publisher = "Springer Nature Link",

pages = "259--260",

editor = "A. Moitinho and J. Alves",

booktitle = "Star Clusters in the Era of Large Surveys",

address = "Netherlands",

note = "5th JENAM Symposium ; Conference date: 09-09-2010 Through 10-09-2010",

}

Raddi, R, Drew, JE, Sale, SE & Steeghs, DTH 2012, Tracing the structure of the Perseus arm with IPHAS. in A Moitinho & J Alves (eds), Star Clusters in the Era of Large Surveys: Proceedings of Symposium 5 of JENAM 2010. Astrophysics and Space Science Proceedings, Springer Nature Link, pp. 259-260, 5th JENAM Symposium, Portugal, 9/09/10. https://doi.org/10.1007/978-3-642-22113-2_48

Tracing the structure of the Perseus arm with IPHAS. / Raddi, Roberto; Drew, J.E.; Sale, S.E. et al.
Star Clusters in the Era of Large Surveys: Proceedings of Symposium 5 of JENAM 2010. ed. / A. Moitinho; J. Alves. Springer Nature Link, 2012. p. 259-260 (Astrophysics and Space Science Proceedings).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

TY - GEN

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AU - Sale, S.E.

AU - Steeghs, D.T.H.

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N2 - Research aiming to describe the spiral structure of the Milky Way disc has to confront both difficulties in obtaining distances and the high interstellar extinction found in the Galactic plane. We present a study of a section of the Perseus Arm, between Galactic longitudes. (120°, 140°) and Galactic latitudes .(-1°+4°), including a number of young clusters. Determination of physical parameters of young stellar objects (YSO) and mapping of the A-star surface density are used to analyse evidence of young structures (typically 10-100 Myrs old) defined in space

AB - Research aiming to describe the spiral structure of the Milky Way disc has to confront both difficulties in obtaining distances and the high interstellar extinction found in the Galactic plane. We present a study of a section of the Perseus Arm, between Galactic longitudes. (120°, 140°) and Galactic latitudes .(-1°+4°), including a number of young clusters. Determination of physical parameters of young stellar objects (YSO) and mapping of the A-star surface density are used to analyse evidence of young structures (typically 10-100 Myrs old) defined in space

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DO - 10.1007/978-3-642-22113-2_48

M3 - Conference contribution

AN - SCOPUS:84896463167

SN - 978-364222112-5

T3 - Astrophysics and Space Science Proceedings

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BT - Star Clusters in the Era of Large Surveys

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PB - Springer Nature Link

T2 - 5th JENAM Symposium

Y2 - 9 September 2010 through 10 September 2010

ER -

Tracing the structure of the Perseus arm with IPHAS

Abstract

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