University of Hertfordshire

By the same authors

Star and Stellar Cluster Formation: ALMA-SKA Synergies

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

Standard

Star and Stellar Cluster Formation: ALMA-SKA Synergies. / Forbrich, Jan; Rathbone, J.; Fuller, G.; Longmore, S.; Molinari, S.

Proceedings of Advancing Astrophysics with the Square Kilometre Array (AASKA14). 2015.

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

Harvard

Forbrich, J, Rathbone, J, Fuller, G, Longmore, S & Molinari, S 2015, Star and Stellar Cluster Formation: ALMA-SKA Synergies. in Proceedings of Advancing Astrophysics with the Square Kilometre Array (AASKA14). Advancing Astrophysics with the Square Kilometre Array, Giardini Naxos, Italy, 9/06/14. <https://pos.sissa.it/archive/conferences/215/152/AASKA14_152.pdf>

APA

Forbrich, J., Rathbone, J., Fuller, G., Longmore, S., & Molinari, S. (2015). Star and Stellar Cluster Formation: ALMA-SKA Synergies. In Proceedings of Advancing Astrophysics with the Square Kilometre Array (AASKA14) https://pos.sissa.it/archive/conferences/215/152/AASKA14_152.pdf

Vancouver

Forbrich J, Rathbone J, Fuller G, Longmore S, Molinari S. Star and Stellar Cluster Formation: ALMA-SKA Synergies. In Proceedings of Advancing Astrophysics with the Square Kilometre Array (AASKA14). 2015

Author

Forbrich, Jan ; Rathbone, J. ; Fuller, G. ; Longmore, S. ; Molinari, S. / Star and Stellar Cluster Formation: ALMA-SKA Synergies. Proceedings of Advancing Astrophysics with the Square Kilometre Array (AASKA14). 2015.

Bibtex

@inproceedings{465639a24f3d48e5ab6a3bba056e0539,
title = "Star and Stellar Cluster Formation: ALMA-SKA Synergies",
abstract = "Over the next decade, observations conducted with ALMA and the SKA will reveal the process of mass assembly and accretion onto young stars and will be revolutionary for studies of star formation. Here we summarise the capabilities of ALMA and discuss recent results from its early science observations. We then review infrared and radio variability observations of both young low-mass and high-mass stars. A time domain SKA radio continuum survey of star forming regions is then outlined. This survey will produce radio light-curves for hundreds of young sources, providing for the first time a systematic survey of radio variability across the full range of stellar masses. These light-curves will probe the magnetospheric interactions of young binary systems, the origins of outflows, trace episodic accretion on the central sources and potentially constrain the rotation rates of embedded sources.",
keywords = "Astrophysics, Astrophysics of galaxies, Astrophysics - Solar and Stellar Astrophysics",
author = "Jan Forbrich and J. Rathbone and G. Fuller and S. Longmore and S. Molinari",
note = "{\textcopyright} 2015 The Author(s). This work is made available under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike license https://creativecommons.org/licenses/by-nc-sa/3.0/.; Advancing Astrophysics with the Square Kilometre Array, AASKA14 ; Conference date: 09-06-2014 Through 13-06-2014",
year = "2015",
month = apr,
language = "English",
booktitle = "Proceedings of Advancing Astrophysics with the Square Kilometre Array (AASKA14)",

}

RIS

TY - GEN

T1 - Star and Stellar Cluster Formation: ALMA-SKA Synergies

AU - Forbrich, Jan

AU - Rathbone, J.

AU - Fuller, G.

AU - Longmore, S.

AU - Molinari, S.

N1 - Conference code: c14-06-09.8

PY - 2015/4

Y1 - 2015/4

N2 - Over the next decade, observations conducted with ALMA and the SKA will reveal the process of mass assembly and accretion onto young stars and will be revolutionary for studies of star formation. Here we summarise the capabilities of ALMA and discuss recent results from its early science observations. We then review infrared and radio variability observations of both young low-mass and high-mass stars. A time domain SKA radio continuum survey of star forming regions is then outlined. This survey will produce radio light-curves for hundreds of young sources, providing for the first time a systematic survey of radio variability across the full range of stellar masses. These light-curves will probe the magnetospheric interactions of young binary systems, the origins of outflows, trace episodic accretion on the central sources and potentially constrain the rotation rates of embedded sources.

AB - Over the next decade, observations conducted with ALMA and the SKA will reveal the process of mass assembly and accretion onto young stars and will be revolutionary for studies of star formation. Here we summarise the capabilities of ALMA and discuss recent results from its early science observations. We then review infrared and radio variability observations of both young low-mass and high-mass stars. A time domain SKA radio continuum survey of star forming regions is then outlined. This survey will produce radio light-curves for hundreds of young sources, providing for the first time a systematic survey of radio variability across the full range of stellar masses. These light-curves will probe the magnetospheric interactions of young binary systems, the origins of outflows, trace episodic accretion on the central sources and potentially constrain the rotation rates of embedded sources.

KW - Astrophysics

KW - Astrophysics of galaxies

KW - Astrophysics - Solar and Stellar Astrophysics

M3 - Conference contribution

BT - Proceedings of Advancing Astrophysics with the Square Kilometre Array (AASKA14)

T2 - Advancing Astrophysics with the Square Kilometre Array

Y2 - 9 June 2014 through 13 June 2014

ER -