University of Hertfordshire

Tracing the structure of the Perseus arm with IPHAS

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Standard

Tracing the structure of the Perseus arm with IPHAS. / Raddi, Roberto; Drew, J.E.; Sale, S.E.; Steeghs, D.T.H.

Star Clusters in the Era of Large Surveys: Proceedings of Symposium 5 of JENAM 2010. ed. / A. Moitinho; J. Alves. Springer, 2012. p. 259-260 (Astrophysics and Space Science Proceedings).

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Harvard

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, pp. 259-260, 5th JENAM Symposium, Portugal, 9/09/10. https://doi.org/10.1007/978-3-642-22113-2_48

APA

Raddi, R., Drew, J. E., Sale, S. E., & Steeghs, D. T. H. (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 (pp. 259-260). (Astrophysics and Space Science Proceedings). Springer. https://doi.org/10.1007/978-3-642-22113-2_48

Vancouver

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

Author

Raddi, Roberto ; Drew, J.E. ; Sale, S.E. ; Steeghs, D.T.H. / Tracing the structure of the Perseus arm with IPHAS. Star Clusters in the Era of Large Surveys: Proceedings of Symposium 5 of JENAM 2010. editor / A. Moitinho ; J. Alves. Springer, 2012. pp. 259-260 (Astrophysics and Space Science Proceedings).

Bibtex

@inproceedings{8bcbd30a996142b4a8e0aa808573d05b,
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",
pages = "259--260",
editor = "A. Moitinho and J. Alves",
booktitle = "Star Clusters in the Era of Large Surveys",

}

RIS

TY - GEN

T1 - Tracing the structure of the Perseus arm with IPHAS

AU - Raddi, Roberto

AU - Drew, J.E.

AU - Sale, S.E.

AU - Steeghs, D.T.H.

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

U2 - 10.1007/978-3-642-22113-2_48

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

SP - 259

EP - 260

BT - Star Clusters in the Era of Large Surveys

A2 - Moitinho, A.

A2 - Alves, J.

PB - Springer

ER -