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The GALAH+ survey : a new library of observed stellar spectra improves radial velocities and hints at motions within M67
ID
Zwitter, Tomaž
(
Author
),
ID
Kos, Janez
(
Author
),
ID
Čotar, Klemen
(
Author
),
ID
Beeson, Kevin Luke
(
Author
),
ID
Vogrinčič, Rok
(
Author
), et al.
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https://academic.oup.com/mnras/article/508/3/4202/6372926
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Abstract
GALAH+ is a magnitude-limited survey of high-resolution stellar spectra obtained by the HERMES spectrograph at the Australian Astronomical Observatory. Its third data release provides reduced spectra with new derivations of stellar parameters and abundances of 30 chemical elements for 584 015 dwarfs and giants, 88 per cent of them in the Gaia magnitude range 11 < G < 14. Here, we use these improved values of stellar parameters to build a library of observed spectra which is useful to study variations of individual spectral lines with stellar parameters. This and other improvements are used to derive radial velocities with uncertainties which are generally within 0.1 km s$^{−1}$ or ∼25 per cent smaller than in the previous release. Median differences in radial velocities measured here and by the Gaia DR2 or APOGEE DR16 surveys are smaller than 30 m s$^{−1}$, a larger offset is present only for Gaia measurements of giant stars. We identify 4483 stars with intrinsically variable velocities and 225 stars for which the velocity stays constant over ≥3 visits spanning more than a year. The combination of radial velocities from GALAH+ with distances and sky plane motions from Gaia enables studies of dynamics within streams and clusters. For example, we estimate that the open cluster M67 has a total mass of ∼3300 M$_⊙$ and its outer parts seem to be expanding, though astrometry with a larger time-span than currently available from Gaia eDR3 is needed to judge if the latter result is real.
Language:
English
Keywords:
Galaxy
,
spectroscopy
,
kinematics
,
dynamics
,
methods
,
data analysis
,
surveys
,
stars
,
fundamental parameters
,
open clusters and associations
,
individual stars
,
M67
Work type:
Article
Typology:
1.01 - Original Scientific Article
Organization:
FMF - Faculty of Mathematics and Physics
Publication status:
Published
Publication version:
Version of Record
Year:
2021
Number of pages:
Str. 4202-4215
Numbering:
Vol. 508, iss. 3
PID:
20.500.12556/RUL-141911
UDC:
524.3
ISSN on article:
1365-2966
DOI:
10.1093/mnras/stab2673
COBISS.SI-ID:
83933187
Publication date in RUL:
11.10.2022
Views:
657
Downloads:
99
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Record is a part of a journal
Title:
Monthly notices of the Royal Astronomical Society
Shortened title:
Mon. not. R. Astron. Soc.
Publisher:
Blackwell Science
ISSN:
1365-2966
COBISS.SI-ID:
1870180
Licences
License:
CC BY 4.0, Creative Commons Attribution 4.0 International
Link:
http://creativecommons.org/licenses/by/4.0/
Description:
This is the standard Creative Commons license that gives others maximum freedom to do what they want with the work as long as they credit the author.
Projects
Funder:
ARRS - Slovenian Research Agency
Project number:
P1-0188
Name:
Astrofizika in fizika atmosfere
Funder:
Other - Other funder or multiple funders
Funding programme:
European Space Agency, Prodex Experiment Arrangement
Project number:
C4000127986
Funder:
ARC - Australian Research Council
Funding programme:
Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)
Project number:
CE170100013
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