Overview of the Massive Young Star-Forming Complex Study in Infrared and X-ray (MYStIX) project

Eric D. Feigelson, Leisa K. Townsley, Patrick S. Broos, Heather A. Busk, Konstantin V. Getman, Robert R. King, Michael A. Kuhn, Tim Naylor, Matthew S. Povich, Adrian Baddeley, Matthew R. Bate, Remy Indebetouw, Kevin L. Luhman, Mark J. McCaughrean, Julian M. Pittard, Ralph E. Pudritz, Alison Sills, Yong Song, James Wadsley

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Abstract

The Massive Young Star-Forming Complex Study in Infrared and X-ray (MYStIX) seeks to characterize 20 OB-dominated young clusters and their environs at distances d ≤ 4 kpc using imaging detectors on the Chandra X-ray Observatory, Spitzer Space Telescope, and the United Kingdom InfraRed Telescope. The observational goals are to construct catalogs of star-forming complex stellar members with well-defined criteria and maps of nebular gas (particularly of hot X-ray-emitting plasma) and dust. A catalog of MYStIX Probable Complex Members with several hundred OB stars and 31,784 low-mass pre-main sequence stars is assembled. This sample and related data products will be used to seek new empirical constraints on theoretical models of cluster formation and dynamics, mass segregation, OB star formation, star formation triggering on the periphery of H II regions, and the survivability of protoplanetary disks in H II regions. This paper gives an introduction and overview of the project, covering the data analysis methodology and application to two star-forming regions: NGC 2264 and the Trifid Nebula.

Original languageEnglish (US)
Article number26
JournalAstrophysical Journal, Supplement Series
Volume209
Issue number2
DOIs
StatePublished - Dec 1 2013

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stars
H II regions
x rays
catalogs
star formation
pre-main sequence stars
infrared telescopes
data products
Space Infrared Telescope Facility
United Kingdom
protoplanetary disks
nebulae
observatory
dust
observatories
plasma
coverings
methodology
project
young

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Feigelson, Eric D. ; Townsley, Leisa K. ; Broos, Patrick S. ; Busk, Heather A. ; Getman, Konstantin V. ; King, Robert R. ; Kuhn, Michael A. ; Naylor, Tim ; Povich, Matthew S. ; Baddeley, Adrian ; Bate, Matthew R. ; Indebetouw, Remy ; Luhman, Kevin L. ; McCaughrean, Mark J. ; Pittard, Julian M. ; Pudritz, Ralph E. ; Sills, Alison ; Song, Yong ; Wadsley, James. / Overview of the Massive Young Star-Forming Complex Study in Infrared and X-ray (MYStIX) project. In: Astrophysical Journal, Supplement Series. 2013 ; Vol. 209, No. 2.
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abstract = "The Massive Young Star-Forming Complex Study in Infrared and X-ray (MYStIX) seeks to characterize 20 OB-dominated young clusters and their environs at distances d ≤ 4 kpc using imaging detectors on the Chandra X-ray Observatory, Spitzer Space Telescope, and the United Kingdom InfraRed Telescope. The observational goals are to construct catalogs of star-forming complex stellar members with well-defined criteria and maps of nebular gas (particularly of hot X-ray-emitting plasma) and dust. A catalog of MYStIX Probable Complex Members with several hundred OB stars and 31,784 low-mass pre-main sequence stars is assembled. This sample and related data products will be used to seek new empirical constraints on theoretical models of cluster formation and dynamics, mass segregation, OB star formation, star formation triggering on the periphery of H II regions, and the survivability of protoplanetary disks in H II regions. This paper gives an introduction and overview of the project, covering the data analysis methodology and application to two star-forming regions: NGC 2264 and the Trifid Nebula.",
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Feigelson, ED, Townsley, LK, Broos, PS, Busk, HA, Getman, KV, King, RR, Kuhn, MA, Naylor, T, Povich, MS, Baddeley, A, Bate, MR, Indebetouw, R, Luhman, KL, McCaughrean, MJ, Pittard, JM, Pudritz, RE, Sills, A, Song, Y & Wadsley, J 2013, 'Overview of the Massive Young Star-Forming Complex Study in Infrared and X-ray (MYStIX) project', Astrophysical Journal, Supplement Series, vol. 209, no. 2, 26. https://doi.org/10.1088/0067-0049/209/2/26

Overview of the Massive Young Star-Forming Complex Study in Infrared and X-ray (MYStIX) project. / Feigelson, Eric D.; Townsley, Leisa K.; Broos, Patrick S.; Busk, Heather A.; Getman, Konstantin V.; King, Robert R.; Kuhn, Michael A.; Naylor, Tim; Povich, Matthew S.; Baddeley, Adrian; Bate, Matthew R.; Indebetouw, Remy; Luhman, Kevin L.; McCaughrean, Mark J.; Pittard, Julian M.; Pudritz, Ralph E.; Sills, Alison; Song, Yong; Wadsley, James.

In: Astrophysical Journal, Supplement Series, Vol. 209, No. 2, 26, 01.12.2013.

Research output: Contribution to journalArticle

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AU - Feigelson, Eric D.

AU - Townsley, Leisa K.

AU - Broos, Patrick S.

AU - Busk, Heather A.

AU - Getman, Konstantin V.

AU - King, Robert R.

AU - Kuhn, Michael A.

AU - Naylor, Tim

AU - Povich, Matthew S.

AU - Baddeley, Adrian

AU - Bate, Matthew R.

AU - Indebetouw, Remy

AU - Luhman, Kevin L.

AU - McCaughrean, Mark J.

AU - Pittard, Julian M.

AU - Pudritz, Ralph E.

AU - Sills, Alison

AU - Song, Yong

AU - Wadsley, James

PY - 2013/12/1

Y1 - 2013/12/1

N2 - The Massive Young Star-Forming Complex Study in Infrared and X-ray (MYStIX) seeks to characterize 20 OB-dominated young clusters and their environs at distances d ≤ 4 kpc using imaging detectors on the Chandra X-ray Observatory, Spitzer Space Telescope, and the United Kingdom InfraRed Telescope. The observational goals are to construct catalogs of star-forming complex stellar members with well-defined criteria and maps of nebular gas (particularly of hot X-ray-emitting plasma) and dust. A catalog of MYStIX Probable Complex Members with several hundred OB stars and 31,784 low-mass pre-main sequence stars is assembled. This sample and related data products will be used to seek new empirical constraints on theoretical models of cluster formation and dynamics, mass segregation, OB star formation, star formation triggering on the periphery of H II regions, and the survivability of protoplanetary disks in H II regions. This paper gives an introduction and overview of the project, covering the data analysis methodology and application to two star-forming regions: NGC 2264 and the Trifid Nebula.

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