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Science Results from the VISTA Survey of the Orion Star-forming Region

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Science Results from the VISTA Survey of the Orion Star-forming Region. / Petr-Gotzens, M.; Alcalá, J. M.; Briceño, C.; González-Solares, E.; Spezzi, L.; Teixeira, P.; Osorio, M. R. Z.; Comerón, F.; Emerson, J.; Hodgkin, S.; Hussain, G.; McCaughrean, M.; Melnick, J.; Oliveira, J.; Ramsay, S.; Stanke, T.; Winston, E.; Zinnecker, H.

In: The Messenger, Vol. 145, 01.09.2011, p. 29-32.

Research output: Contribution to journalArticlepeer-review

Harvard

Petr-Gotzens, M, Alcalá, JM, Briceño, C, González-Solares, E, Spezzi, L, Teixeira, P, Osorio, MRZ, Comerón, F, Emerson, J, Hodgkin, S, Hussain, G, McCaughrean, M, Melnick, J, Oliveira, J, Ramsay, S, Stanke, T, Winston, E & Zinnecker, H 2011, 'Science Results from the VISTA Survey of the Orion Star-forming Region', The Messenger, vol. 145, pp. 29-32. <http://adsabs.harvard.edu/abs/2011Msngr.145...29P>

APA

Petr-Gotzens, M., Alcalá, J. M., Briceño, C., González-Solares, E., Spezzi, L., Teixeira, P., Osorio, M. R. Z., Comerón, F., Emerson, J., Hodgkin, S., Hussain, G., McCaughrean, M., Melnick, J., Oliveira, J., Ramsay, S., Stanke, T., Winston, E., & Zinnecker, H. (2011). Science Results from the VISTA Survey of the Orion Star-forming Region. The Messenger, 145, 29-32. http://adsabs.harvard.edu/abs/2011Msngr.145...29P

Vancouver

Petr-Gotzens M, Alcalá JM, Briceño C, González-Solares E, Spezzi L, Teixeira P et al. Science Results from the VISTA Survey of the Orion Star-forming Region. The Messenger. 2011 Sep 1;145:29-32.

Author

Petr-Gotzens, M. ; Alcalá, J. M. ; Briceño, C. ; González-Solares, E. ; Spezzi, L. ; Teixeira, P. ; Osorio, M. R. Z. ; Comerón, F. ; Emerson, J. ; Hodgkin, S. ; Hussain, G. ; McCaughrean, M. ; Melnick, J. ; Oliveira, J. ; Ramsay, S. ; Stanke, T. ; Winston, E. ; Zinnecker, H. / Science Results from the VISTA Survey of the Orion Star-forming Region. In: The Messenger. 2011 ; Vol. 145. pp. 29-32.

Bibtex - Download

@article{14bd35b7afed4e5d92053fa279d178c2,
title = "Science Results from the VISTA Survey of the Orion Star-forming Region",
abstract = "As part of the VISTA Science Verification programme, a large set of images in Orion was obtained at five near-infrared wavelength bands, from 0.9 to 2.2 μm. The resulting multi-band catalogue contains approximately three million sources, allowing investigation of various issues concerning star and brown dwarf formation, such as a) the difference in the shape of the substellar mass function in a cluster vs. non-clustered environment, b) the influence of massive OB stars on the process of brown dwarf formation, c) the size and morphology of dust envelopes around protostars, and d) the comparative role of mass and environment on the evolution of circumstellar discs. The data from the VISTA Orion Survey, including catalogues, are available to the community. In this article we present an overview of selected science results that have emerged so far from this survey.",
author = "M. Petr-Gotzens and Alcal{\'a}, {J. M.} and C. Brice{\~n}o and E. Gonz{\'a}lez-Solares and L. Spezzi and P. Teixeira and Osorio, {M. R. Z.} and F. Comer{\'o}n and J. Emerson and S. Hodgkin and G. Hussain and M. McCaughrean and J. Melnick and J. Oliveira and S. Ramsay and T. Stanke and E. Winston and H. Zinnecker",
year = "2011",
month = sep,
day = "1",
language = "English",
volume = "145",
pages = "29--32",
journal = "The Messenger",
issn = "0722-6691",

}

RIS (suitable for import to EndNote) - Download

TY - JOUR

T1 - Science Results from the VISTA Survey of the Orion Star-forming Region

AU - Petr-Gotzens, M.

AU - Alcalá, J. M.

AU - Briceño, C.

AU - González-Solares, E.

AU - Spezzi, L.

AU - Teixeira, P.

AU - Osorio, M. R. Z.

AU - Comerón, F.

AU - Emerson, J.

AU - Hodgkin, S.

AU - Hussain, G.

AU - McCaughrean, M.

AU - Melnick, J.

AU - Oliveira, J.

AU - Ramsay, S.

AU - Stanke, T.

AU - Winston, E.

AU - Zinnecker, H.

PY - 2011/9/1

Y1 - 2011/9/1

N2 - As part of the VISTA Science Verification programme, a large set of images in Orion was obtained at five near-infrared wavelength bands, from 0.9 to 2.2 μm. The resulting multi-band catalogue contains approximately three million sources, allowing investigation of various issues concerning star and brown dwarf formation, such as a) the difference in the shape of the substellar mass function in a cluster vs. non-clustered environment, b) the influence of massive OB stars on the process of brown dwarf formation, c) the size and morphology of dust envelopes around protostars, and d) the comparative role of mass and environment on the evolution of circumstellar discs. The data from the VISTA Orion Survey, including catalogues, are available to the community. In this article we present an overview of selected science results that have emerged so far from this survey.

AB - As part of the VISTA Science Verification programme, a large set of images in Orion was obtained at five near-infrared wavelength bands, from 0.9 to 2.2 μm. The resulting multi-band catalogue contains approximately three million sources, allowing investigation of various issues concerning star and brown dwarf formation, such as a) the difference in the shape of the substellar mass function in a cluster vs. non-clustered environment, b) the influence of massive OB stars on the process of brown dwarf formation, c) the size and morphology of dust envelopes around protostars, and d) the comparative role of mass and environment on the evolution of circumstellar discs. The data from the VISTA Orion Survey, including catalogues, are available to the community. In this article we present an overview of selected science results that have emerged so far from this survey.

M3 - Article

VL - 145

SP - 29

EP - 32

JO - The Messenger

JF - The Messenger

SN - 0722-6691

ER -

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