The tricky line of sight towards Cygnus-X: The [DB2001] CL05 embedded cluster as a pilot case

D. de la Fuente; C. G. Román-Zúñiga; E. Jiménez-Bailón; J. Alves; S. Venus

The tricky line of sight towards Cygnus-X: The [DB2001] CL05 embedded cluster as a pilot case

D. de la Fuente
, C. G. Román-Zúñiga
, E. Jiménez-Bailón
, J. Alves
, S. Venus

Department of Astrophysics

Publications: Contribution to book › Contribution to proceedings

Abstract

The nearest massive star-forming complex, Cygnus-X, is widely used as a laboratory for star cluster formation and feedback processes, under the implicit assumption that all its components are located roughly at the same distance. We present a multi-wavelength study of a 15' × 15' field in southern Cygnus-X, where different components involving clustered star formation are overlapped. Preliminary results indicate that the Berkeley 87 and [DB2001] CL05 clusters are actually located at very different distances, invalidating previous claims of physical interaction between them. This shows the importance of a careful treatment of extinction and distance calculations for cluster formation studies, particularly in Cygnus-X.

Original language	English
Title of host publication	Highlights on Spanish Astrophysics X
Subtitle of host publication	Proceedings of the XIII Scientific Meeting of the Spanish Astronomical Society held on July 16-20, 2018, in Salamanca, Spain
Editors	B. Montesinos
Pages	296-301
Publication status	Published - Mar 2019
Event	XIII Sientific Meeting of the Spanish Astronomical Society - Salamanca, Spain Duration: 16 Jul 2018 → 20 Jul 2018

Conference

Conference	XIII Sientific Meeting of the Spanish Astronomical Society
Country/Territory	Spain
City	Salamanca
Period	16/07/18 → 20/07/18

Austrian Fields of Science 2012

103003 Astronomy
103004 Astrophysics

Access to Document

http://adsabs.harvard.edu/abs/2019hsax.conf..296D

Cite this

de la Fuente, D., Román-Zúñiga, C. G., Jiménez-Bailón, E., Alves, J., & Venus, S. (2019). The tricky line of sight towards Cygnus-X: The [DB2001] CL05 embedded cluster as a pilot case. In B. Montesinos (Ed.), Highlights on Spanish Astrophysics X: Proceedings of the XIII Scientific Meeting of the Spanish Astronomical Society held on July 16-20, 2018, in Salamanca, Spain (pp. 296-301) http://adsabs.harvard.edu/abs/2019hsax.conf..296D

de la Fuente, D. ; Román-Zúñiga, C. G. ; Jiménez-Bailón, E. et al. / The tricky line of sight towards Cygnus-X: The [DB2001] CL05 embedded cluster as a pilot case. Highlights on Spanish Astrophysics X: Proceedings of the XIII Scientific Meeting of the Spanish Astronomical Society held on July 16-20, 2018, in Salamanca, Spain. editor / B. Montesinos. 2019. pp. 296-301

@inproceedings{e5d81419d6844a90afb42df356da1577,

title = "The tricky line of sight towards Cygnus-X: The [DB2001] CL05 embedded cluster as a pilot case",

abstract = "The nearest massive star-forming complex, Cygnus-X, is widely used as a laboratory for star cluster formation and feedback processes, under the implicit assumption that all its components are located roughly at the same distance. We present a multi-wavelength study of a 15' × 15' field in southern Cygnus-X, where different components involving clustered star formation are overlapped. Preliminary results indicate that the Berkeley 87 and [DB2001] CL05 clusters are actually located at very different distances, invalidating previous claims of physical interaction between them. This shows the importance of a careful treatment of extinction and distance calculations for cluster formation studies, particularly in Cygnus-X.",

author = "\{de la Fuente\}, D. and Rom{\'a}n-Z{\'u}{\~n}iga, \{C. G.\} and E. Jim{\'e}nez-Bail{\'o}n and J. Alves and S. Venus",

year = "2019",

month = mar,

language = "English",

isbn = "978-84-09-09331-1",

pages = "296--301",

editor = "B. Montesinos",

booktitle = "Highlights on Spanish Astrophysics X",

note = "XIII Sientific Meeting of the Spanish Astronomical Society ; Conference date: 16-07-2018 Through 20-07-2018",

}

de la Fuente, D, Román-Zúñiga, CG, Jiménez-Bailón, E, Alves, J & Venus, S 2019, The tricky line of sight towards Cygnus-X: The [DB2001] CL05 embedded cluster as a pilot case. in B Montesinos (ed.), Highlights on Spanish Astrophysics X: Proceedings of the XIII Scientific Meeting of the Spanish Astronomical Society held on July 16-20, 2018, in Salamanca, Spain. pp. 296-301, XIII Sientific Meeting of the Spanish Astronomical Society, Salamanca, Spain, 16/07/18. <http://adsabs.harvard.edu/abs/2019hsax.conf..296D>

The tricky line of sight towards Cygnus-X: The [DB2001] CL05 embedded cluster as a pilot case. / de la Fuente, D.; Román-Zúñiga, C. G.; Jiménez-Bailón, E. et al.
Highlights on Spanish Astrophysics X: Proceedings of the XIII Scientific Meeting of the Spanish Astronomical Society held on July 16-20, 2018, in Salamanca, Spain. ed. / B. Montesinos. 2019. p. 296-301.

Publications: Contribution to book › Contribution to proceedings

TY - GEN

T1 - The tricky line of sight towards Cygnus-X: The [DB2001] CL05 embedded cluster as a pilot case

AU - de la Fuente, D.

AU - Román-Zúñiga, C. G.

AU - Jiménez-Bailón, E.

AU - Alves, J.

AU - Venus, S.

PY - 2019/3

Y1 - 2019/3

N2 - The nearest massive star-forming complex, Cygnus-X, is widely used as a laboratory for star cluster formation and feedback processes, under the implicit assumption that all its components are located roughly at the same distance. We present a multi-wavelength study of a 15' × 15' field in southern Cygnus-X, where different components involving clustered star formation are overlapped. Preliminary results indicate that the Berkeley 87 and [DB2001] CL05 clusters are actually located at very different distances, invalidating previous claims of physical interaction between them. This shows the importance of a careful treatment of extinction and distance calculations for cluster formation studies, particularly in Cygnus-X.

AB - The nearest massive star-forming complex, Cygnus-X, is widely used as a laboratory for star cluster formation and feedback processes, under the implicit assumption that all its components are located roughly at the same distance. We present a multi-wavelength study of a 15' × 15' field in southern Cygnus-X, where different components involving clustered star formation are overlapped. Preliminary results indicate that the Berkeley 87 and [DB2001] CL05 clusters are actually located at very different distances, invalidating previous claims of physical interaction between them. This shows the importance of a careful treatment of extinction and distance calculations for cluster formation studies, particularly in Cygnus-X.

M3 - Contribution to proceedings

SN - 978-84-09-09331-1

SP - 296

EP - 301

BT - Highlights on Spanish Astrophysics X

A2 - Montesinos, B.

T2 - XIII Sientific Meeting of the Spanish Astronomical Society

Y2 - 16 July 2018 through 20 July 2018

ER -

de la Fuente D, Román-Zúñiga CG, Jiménez-Bailón E, Alves J, Venus S. The tricky line of sight towards Cygnus-X: The [DB2001] CL05 embedded cluster as a pilot case. In Montesinos B, editor, Highlights on Spanish Astrophysics X: Proceedings of the XIII Scientific Meeting of the Spanish Astronomical Society held on July 16-20, 2018, in Salamanca, Spain. 2019. p. 296-301

The tricky line of sight towards Cygnus-X: The [DB2001] CL05 embedded cluster as a pilot case

Abstract

Conference

Austrian Fields of Science 2012

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