Benchmark low-mass objects in Moving Groups

M. C. Galvez-Ortiz; M. Kuznetsov; J. R. A. Clarke; Ya. V. Pavlenko; D.J. Pinfield; H.R.A. Jones; J. S. Jenkins; J. Barnes; B. Burningham; A. C. Day-Jones; E. L. Martin; A. E. Garcia Perez; R.S. Pokorny

doi:10.1051/epjconf/20134705007

Benchmark low-mass objects in Moving Groups

M. C. Galvez-Ortiz, M. Kuznetsov, J. R. A. Clarke, Ya. V. Pavlenko, D.J. Pinfield, H.R.A. Jones, J. S. Jenkins, J. Barnes, B. Burningham, A. C. Day-Jones, E. L. Martin, A. E. Garcia Perez, R.S. Pokorny

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

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Abstract

In order to compile a sample of ultracool dwarfs that will serve as benchmarks for testing theoretical formation and evolutionary models, we selected low-mass cool (>M7) objects that are potentially members of five known young Moving Groups in the solar neighbourhood.

We have studied the kinematics of the sample, finding that 49 targets belong to the young disk area, from which 36 are kinematic member of one of the five moving groups under study. Some of the identified low-mass members have been spectroscopically characterised (T-eff, log g) and confirmed as young members through a detailed study of age indicators.

Original language	English
Title of host publication	Hot Planets and Cool Stars
Editors	R. Saglia
Publisher	EDP Sciences
Number of pages	4
DOIs	https://doi.org/10.1051/epjconf/20134705007
Publication status	Published - 2013
Event	Conference on Hot Planets and Cool Stars - Garching, Germany Duration: 12 Nov 2012 → 16 Nov 2012

Publication series

Name	EPJ Web of Conferences
Volume	47
ISSN (Print)	2100-014X

Conference

Conference	Conference on Hot Planets and Cool Stars
Country/Territory	Germany
Period	12/11/12 → 16/11/12

Keywords

BROWN DWARFS
STARS
SPECTROSCOPY
VELOCITIES
MEMBERS
SEARCH

Access to Document

10.1051/epjconf/20134705007

906843
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 2.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited
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Galvez-Ortiz, M. C., Kuznetsov, M., Clarke, J. R. A., Pavlenko, Y. V., Pinfield, D. J., Jones, H. R. A., Jenkins, J. S., Barnes, J., Burningham, B., Day-Jones, A. C., Martin, E. L., Perez, A. E. G., & Pokorny, R. S. (2013). Benchmark low-mass objects in Moving Groups. In R. Saglia (Ed.), Hot Planets and Cool Stars Article 05007 (EPJ Web of Conferences; Vol. 47). EDP Sciences. https://doi.org/10.1051/epjconf/20134705007

@inproceedings{2c4067d4cca9425795cd31387de3301b,

title = "Benchmark low-mass objects in Moving Groups",

abstract = "In order to compile a sample of ultracool dwarfs that will serve as benchmarks for testing theoretical formation and evolutionary models, we selected low-mass cool (>M7) objects that are potentially members of five known young Moving Groups in the solar neighbourhood. We have studied the kinematics of the sample, finding that 49 targets belong to the young disk area, from which 36 are kinematic member of one of the five moving groups under study. Some of the identified low-mass members have been spectroscopically characterised (T-eff, log g) and confirmed as young members through a detailed study of age indicators.",

keywords = "BROWN DWARFS, STARS, SPECTROSCOPY, VELOCITIES, MEMBERS, SEARCH",

author = "Galvez-Ortiz, {M. C.} and M. Kuznetsov and Clarke, {J. R. A.} and Pavlenko, {Ya. V.} and D.J. Pinfield and H.R.A. Jones and Jenkins, {J. S.} and J. Barnes and B. Burningham and Day-Jones, {A. C.} and Martin, {E. L.} and Perez, {A. E. Garcia} and R.S. Pokorny",

note = "This is an Open Access article distributed under the terms of the Creative Commons Attribution License 2.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.; Conference on Hot Planets and Cool Stars ; Conference date: 12-11-2012 Through 16-11-2012",

year = "2013",

doi = "10.1051/epjconf/20134705007",

language = "English",

series = "EPJ Web of Conferences",

publisher = "EDP Sciences",

editor = "R. Saglia",

booktitle = "Hot Planets and Cool Stars",

address = "France",

}

Galvez-Ortiz, MC, Kuznetsov, M, Clarke, JRA, Pavlenko, YV, Pinfield, DJ , Jones, HRA, Jenkins, JS, Barnes, J, Burningham, B, Day-Jones, AC, Martin, EL, Perez, AEG & Pokorny, RS 2013, Benchmark low-mass objects in Moving Groups. in R Saglia (ed.), Hot Planets and Cool Stars., 05007, EPJ Web of Conferences, vol. 47, EDP Sciences, Conference on Hot Planets and Cool Stars, Germany, 12/11/12. https://doi.org/10.1051/epjconf/20134705007

TY - GEN

T1 - Benchmark low-mass objects in Moving Groups

AU - Galvez-Ortiz, M. C.

AU - Kuznetsov, M.

AU - Clarke, J. R. A.

AU - Pavlenko, Ya. V.

AU - Pinfield, D.J.

AU - Jones, H.R.A.

AU - Jenkins, J. S.

AU - Barnes, J.

AU - Burningham, B.

AU - Day-Jones, A. C.

AU - Martin, E. L.

AU - Perez, A. E. Garcia

AU - Pokorny, R.S.

N1 - This is an Open Access article distributed under the terms of the Creative Commons Attribution License 2.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

PY - 2013

Y1 - 2013

N2 - In order to compile a sample of ultracool dwarfs that will serve as benchmarks for testing theoretical formation and evolutionary models, we selected low-mass cool (>M7) objects that are potentially members of five known young Moving Groups in the solar neighbourhood. We have studied the kinematics of the sample, finding that 49 targets belong to the young disk area, from which 36 are kinematic member of one of the five moving groups under study. Some of the identified low-mass members have been spectroscopically characterised (T-eff, log g) and confirmed as young members through a detailed study of age indicators.

AB - In order to compile a sample of ultracool dwarfs that will serve as benchmarks for testing theoretical formation and evolutionary models, we selected low-mass cool (>M7) objects that are potentially members of five known young Moving Groups in the solar neighbourhood. We have studied the kinematics of the sample, finding that 49 targets belong to the young disk area, from which 36 are kinematic member of one of the five moving groups under study. Some of the identified low-mass members have been spectroscopically characterised (T-eff, log g) and confirmed as young members through a detailed study of age indicators.

KW - BROWN DWARFS

KW - STARS

KW - SPECTROSCOPY

KW - VELOCITIES

KW - MEMBERS

KW - SEARCH

U2 - 10.1051/epjconf/20134705007

DO - 10.1051/epjconf/20134705007

M3 - Conference contribution

T3 - EPJ Web of Conferences

BT - Hot Planets and Cool Stars

A2 - Saglia, R.

PB - EDP Sciences

T2 - Conference on Hot Planets and Cool Stars

Y2 - 12 November 2012 through 16 November 2012

ER -

Benchmark low-mass objects in Moving Groups

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Keywords

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