2016ApJ...823..102C


C.D.S. - SIMBAD4 rel 1.7 - 2020.01.20CET01:12:17

2016ApJ...823..102C - Astrophys. J., 823, 102 (2016/June-1)

Mesa isochrones and stellar tracks (MIST). I solar-scaled models.

CHOI J., DOTTER A., CONROY C., CANTIELLO M., PAXTON B. and JOHNSON B.D.

Abstract (from CDS):

This is the first of a series of papers presenting the Modules for Experiments in Stellar Astrophysics (MESA) Isochrones and Stellar Tracks (MIST) project, a new comprehensive set of stellar evolutionary tracks and isochrones computed using MESA, a state-of-the-art open-source 1D stellar evolution package. In this work, we present models with solar-scaled abundance ratios covering a wide range of ages ( 5\leqslant log(Age) [year]\leqslant 10.3 ), masses ( 0.1\leqslant M/{M}_☉\leqslant 300 ), and metallicities ( -2.0\leqslant [Z/H]\leqslant 0.5 ). The models are self-consistently and continuously evolved from the pre-main sequence (PMS) to the end of hydrogen burning, the white dwarf cooling sequence, or the end of carbon burning, depending on the initial mass. We also provide a grid of models evolved from the PMS to the end of core helium burning for -4.0\leqslant [Z/H]\lt -2.0 . We showcase extensive comparisons with observational constraints as well as with some of the most widely used existing models in the literature. The evolutionary tracks and isochrones can be downloaded from the project website at http://waps.cfa.harvard.edu/MIST/.

Abstract Copyright: © 2016. The American Astronomical Society. All rights reserved.

Journal keyword(s): stars: evolution - stars: general - stars: interiors

Simbad objects: 24

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Number of rows : 24

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 M 31 G 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 10659 1
2 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 9177 1
3 M 33 GiG 01 33 50.904 +30 39 35.79 6.17 6.27 5.72     ~ 5046 1
4 NAME Magellanic Clouds GrG 03 00 -71.0           ~ 5441 1
5 Cl Melotte 22 OpC 03 47 00 +24 07.0           ~ 2924 0
6 V* V1098 Tau TT* 04 14 47.9897419517 +27 52 34.232647358   14.08 11.73 10.95   M1 105 0
7 Cl Melotte 25 OpC 04 26 54.00 +15 52 00.0           ~ 2602 0
8 NAME Tau-Aur Region SFR 04 30 +25.0           ~ 1186 1
9 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 14457 1
10 RMC 136 Cl* 05 38 42.396 -69 06 03.36   9.63 9.50     ~ 1688 2
11 M 37 OpC 05 52 18 +32 33.2   6.19 5.6     ~ 327 2
12 * alf CMa B WD* 06 45 09.3021501316 -16 43 00.716804119   8.41 8.44     DA1.9 491 1
13 NGC 2632 OpC 08 40 24 +19 40.0           ~ 1189 0
14 NGC 2682 OpC 08 51 18 +11 48.0           ~ 1995 0
15 NAME Sex A H2G 10 11 00.5 -04 41 30 12.48 12.13 11.93 11.78   ~ 642 2
16 NAME Lower Centaurus Crux As* 12 19 -57.1           ~ 336 1
17 C 1235-509 GlC 12 38 40.20 -51 09 01.0           ~ 309 0
18 NAME Upper Centaurus Lupus As* 15 24 -41.9           ~ 343 1
19 2MASS J15595050-1944373 EB* 15 59 50.5087554948 -19 44 37.367864195           M4 32 0
20 NAME Upper Sco Association As* 16 12 -23.4           ~ 971 1
21 NAME ASSOC II SCO As* 16 15 -24.2           ~ 1085 1
22 * alf Sco ** 16 29 24.45970 -26 25 55.2094 4.08 2.75 0.91 -0.64 -1.87 M0.5Iab+B3V: 685 1
23 NGC 6791 OpC 19 20 53 +37 46.3   10.52 9.5     ~ 852 0
24 NGC 6819 OpC 19 41 18 +40 11.2   8.21 7.3     ~ 450 0

    Equat.    Gal    SGal    Ecl

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2020.01.20-01:12:17

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