Tracing the structure of the Perseus arm with IPHAS

Roberto Raddi; Janet E. Drew; Stuart E. Sale; Danny Steeghs

doi:10.1007/978-3-642-22113-2-48

Tracing the structure of the Perseus arm with IPHAS

Roberto Raddi, Janet E. Drew, Stuart E. Sale, Danny Steeghs

Research output: Chapter in Book/Report/Conference proceeding › Conference Paper › Research › peer-review

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 - Proceedings of Symposium 5 of JENAM 2010
Publisher	Kluwer Academic Publishers
Pages	259-260
Number of pages	2
ISBN (Print)	9783642221125
DOIs	https://doi.org/10.1007/978-3-642-22113-2-48
Publication status	Published - 2012
Externally published	Yes
Event	5th JENAM Symposium: Star Clusters in the Era of Large Surveys, JENAM 2010 - Lisbon, Portugal Duration: 9 Sept 2010 → 10 Sept 2010

Conference

Conference	5th JENAM Symposium: Star Clusters in the Era of Large Surveys, JENAM 2010
Country/Territory	Portugal
City	Lisbon
Period	9/09/10 → 10/09/10

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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 Drew, {Janet E.} and Sale, {Stuart E.} and Danny Steeghs",

year = "2012",

doi = "10.1007/978-3-642-22113-2-48",

language = "English",

isbn = "9783642221125",

pages = "259--260",

booktitle = "Star Clusters in the Era of Large Surveys - Proceedings of Symposium 5 of JENAM 2010",

publisher = "Kluwer Academic Publishers",

address = "Germany",

note = "5th JENAM Symposium: Star Clusters in the Era of Large Surveys, JENAM 2010 ; Conference date: 09-09-2010 Through 10-09-2010",

}

Raddi, R, Drew, JE, Sale, SE & Steeghs, D 2012, Tracing the structure of the Perseus arm with IPHAS. in Star Clusters in the Era of Large Surveys - Proceedings of Symposium 5 of JENAM 2010. Kluwer Academic Publishers, pp. 259-260, 5th JENAM Symposium: Star Clusters in the Era of Large Surveys, JENAM 2010, Lisbon, Portugal, 9/09/10. https://doi.org/10.1007/978-3-642-22113-2-48

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AU - Raddi, Roberto

AU - Drew, Janet E.

AU - Sale, Stuart E.

AU - Steeghs, Danny

PY - 2012

Y1 - 2012

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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U2 - 10.1007/978-3-642-22113-2-48

DO - 10.1007/978-3-642-22113-2-48

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AN - SCOPUS:84896463167

SN - 9783642221125

SP - 259

EP - 260

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

PB - Kluwer Academic Publishers

T2 - 5th JENAM Symposium: Star Clusters in the Era of Large Surveys, JENAM 2010

Y2 - 9 September 2010 through 10 September 2010

ER -

Tracing the structure of the Perseus arm with IPHAS

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