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VLT/SPHERE- and ALMA-based shape reconstruction of asteroid (3) Juno

Tutkimustuotosvertaisarvioitu

Standard

VLT/SPHERE- and ALMA-based shape reconstruction of asteroid (3) Juno. / Viikinkoski, M.; Kaasalainen, M.; Durech, J.; Carry, B.; Marsset, M.; Fusco, T.; Dumas, C.; Merline, W. J.; Yang, B.; Berthier, J.; Kervella, P.; Vernazza, P.

julkaisussa: Astronomy and Astrophysics, Vuosikerta 581, L3, 01.09.2015.

Tutkimustuotosvertaisarvioitu

Harvard

Viikinkoski, M, Kaasalainen, M, Durech, J, Carry, B, Marsset, M, Fusco, T, Dumas, C, Merline, WJ, Yang, B, Berthier, J, Kervella, P & Vernazza, P 2015, 'VLT/SPHERE- and ALMA-based shape reconstruction of asteroid (3) Juno', Astronomy and Astrophysics, Vuosikerta. 581, L3. https://doi.org/10.1051/0004-6361/201526626

APA

Viikinkoski, M., Kaasalainen, M., Durech, J., Carry, B., Marsset, M., Fusco, T., ... Vernazza, P. (2015). VLT/SPHERE- and ALMA-based shape reconstruction of asteroid (3) Juno. Astronomy and Astrophysics, 581, [L3]. https://doi.org/10.1051/0004-6361/201526626

Vancouver

Viikinkoski M, Kaasalainen M, Durech J, Carry B, Marsset M, Fusco T et al. VLT/SPHERE- and ALMA-based shape reconstruction of asteroid (3) Juno. Astronomy and Astrophysics. 2015 syys 1;581. L3. https://doi.org/10.1051/0004-6361/201526626

Author

Viikinkoski, M. ; Kaasalainen, M. ; Durech, J. ; Carry, B. ; Marsset, M. ; Fusco, T. ; Dumas, C. ; Merline, W. J. ; Yang, B. ; Berthier, J. ; Kervella, P. ; Vernazza, P. / VLT/SPHERE- and ALMA-based shape reconstruction of asteroid (3) Juno. Julkaisussa: Astronomy and Astrophysics. 2015 ; Vuosikerta 581.

Bibtex - Lataa

@article{1815f0d0f63b4998ac889f34526d7066,
title = "VLT/SPHERE- and ALMA-based shape reconstruction of asteroid (3) Juno",
abstract = "We use the recently released Atacama Large Millimeter Array (ALMA) and VLT/SPHERE science verification data, together with earlier adaptive-optics images, stellar occultation, and lightcurve data to model the 3D shape and spin of the large asteroid (3) Juno with the all-data asteroid modelling (ADAM) procedure. These data set limits on the plausible range of shape models, yielding reconstructions suggesting that, despite its large size, Juno has sizable unrounded features moulded by non-gravitational processes such as impacts.",
keywords = "Instrumentation: adaptive optics, Instrumentation: interferometers, Methods: numerical, Minor planets, asteroids: individual: (3) Juno",
author = "M. Viikinkoski and M. Kaasalainen and J. Durech and B. Carry and M. Marsset and T. Fusco and C. Dumas and Merline, {W. J.} and B. Yang and J. Berthier and P. Kervella and P. Vernazza",
year = "2015",
month = "9",
day = "1",
doi = "10.1051/0004-6361/201526626",
language = "English",
volume = "581",
journal = "Astronomy and Astrophysics",
issn = "0004-6361",
publisher = "EDP Sciences",

}

RIS (suitable for import to EndNote) - Lataa

TY - JOUR

T1 - VLT/SPHERE- and ALMA-based shape reconstruction of asteroid (3) Juno

AU - Viikinkoski, M.

AU - Kaasalainen, M.

AU - Durech, J.

AU - Carry, B.

AU - Marsset, M.

AU - Fusco, T.

AU - Dumas, C.

AU - Merline, W. J.

AU - Yang, B.

AU - Berthier, J.

AU - Kervella, P.

AU - Vernazza, P.

PY - 2015/9/1

Y1 - 2015/9/1

N2 - We use the recently released Atacama Large Millimeter Array (ALMA) and VLT/SPHERE science verification data, together with earlier adaptive-optics images, stellar occultation, and lightcurve data to model the 3D shape and spin of the large asteroid (3) Juno with the all-data asteroid modelling (ADAM) procedure. These data set limits on the plausible range of shape models, yielding reconstructions suggesting that, despite its large size, Juno has sizable unrounded features moulded by non-gravitational processes such as impacts.

AB - We use the recently released Atacama Large Millimeter Array (ALMA) and VLT/SPHERE science verification data, together with earlier adaptive-optics images, stellar occultation, and lightcurve data to model the 3D shape and spin of the large asteroid (3) Juno with the all-data asteroid modelling (ADAM) procedure. These data set limits on the plausible range of shape models, yielding reconstructions suggesting that, despite its large size, Juno has sizable unrounded features moulded by non-gravitational processes such as impacts.

KW - Instrumentation: adaptive optics

KW - Instrumentation: interferometers

KW - Methods: numerical

KW - Minor planets, asteroids: individual: (3) Juno

UR - http://www.scopus.com/inward/record.url?scp=84941207014&partnerID=8YFLogxK

U2 - 10.1051/0004-6361/201526626

DO - 10.1051/0004-6361/201526626

M3 - Article

VL - 581

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

SN - 0004-6361

M1 - L3

ER -