2019ApJ...877...49G


Query : 2019ApJ...877...49G

2019ApJ...877...49G - Astrophys. J., 877, 49-49 (2019/May-3)

An infrared census of DUST in Nearby Galaxies with Spitzer (DUSTiNGS). V. The period-luminosity relation for dusty metal-poor AGB stars.

GOLDMAN S.R., BOYER M.L., McQUINN K.B.W., WHITELOCK P.A., McDONALD I., VAN LOON J.T., SKILLMAN E.D., GEHRZ R.D., JAVADI A., SLOAN G.C., JONES O.C., GROENEWEGEN M.A.T. and MENZIES J.W.

Abstract (from CDS):

The survey for DUST in Nearby Galaxies with Spitzer (DUSTiNGS) has identified hundreds of candidate dust-producing asymptotic giant branch (AGB) stars in several nearby metal-poor galaxies. We have obtained multi-epoch follow-up observations for these candidates with the Spitzer Space Telescope and measured their infrared (IR) light curves. This has allowed us to confirm their AGB nature and investigate pulsation behavior at very low metallicity. We have obtained high-confidence pulsation periods for 88 sources in seven galaxies. We have confirmed DUSTiNGS variable star candidates with a 20% success rate and determined the pulsation properties of 19 sources already identified as thermally pulsing AGB stars. We find that the AGB pulsation properties are similar in all galaxies surveyed here, with no discernible difference between the DUSTiNGS galaxies (down to 1.4% solar metallicity; [Fe/H] = -1.85) and the far more metal-rich Magellanic Clouds (up to 50% solar metallicity; [Fe/H] = -0.38). These results strengthen the link between dust production and pulsation in AGB stars and establish the IR period-luminosity relation as a reliable tool (±4%) for determining distances to galaxies, regardless of metallicity.

Abstract Copyright: © 2019. The American Astronomical Society. All rights reserved.

Journal keyword(s): galaxies: dwarf - galaxies: stellar content - infrared: stars - Local Group - stars: AGB and post-AGB - stars: carbon

VizieR on-line data: <Available at CDS (J/ApJ/877/49): table2.dat table3.dat lc/*>

Status at CDS : All or part of tables of objects will not be ingested in SIMBAD.

Simbad objects: 26

goto Full paper

goto View the references in ADS

Number of rows : 26
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 MCG-03-01-015 G 00 01 57.9 -15 27 50   11.50 11.10 10.93   ~ 782 2
2 IC 10 rG 00 20 17.33520 +59 18 13.6480   13.6 9.5     ~ 1185 1
3 NGC 147 GiG 00 33 12.120 +48 30 31.46   12.0 9.5     ~ 720 1
4 NGC 185 Sy2 00 38 57.9400026024 +48 20 15.035874648   9.10 9.2     ~ 840 1
5 M 31 AGN 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 13622 1
6 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 12317 1
7 NAME Andromeda IX G 00 52 53.0 +43 11 45     16.3     ~ 176 1
8 NAME Sculptor Dwarf Galaxy G 01 00 09.4 -33 42 32   9.79 8.6 8.81   ~ 1498 4
9 ULAS J010443.69+020324.3 LP* 01 04 43.690 +02 03 23.95           ~ 4 0
10 IC 1613 GiC 01 04 48.4071 +02 07 10.185   10.42 10.01 9.77   ~ 1316 2
11 ULAS J010457.80+020916.9 LP* 01 04 57.811 +02 09 16.94           ~ 4 0
12 M 33 GiG 01 33 50.8965749232 +30 39 36.630403128 6.17 6.27 5.72     ~ 6226 1
13 NAME Phoenix Dwarf Galaxy Sy1 01 51 06.3 -44 26 41   13.48 13.2 12.69   ~ 575 2
14 MCG-06-07-001 G 02 39 59.3 -34 26 57   9.02 7.4     ~ 1894 1
15 NAME Magellanic Clouds GrG 03 00 -71.0           ~ 7988 0
16 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
17 Z 36-12 H2G 10 00 00.8217342072 +05 20 09.533389560 12.77 12.25 11.89 11.71   ~ 569 0
18 Z 64-73 G 10 08 28.12 +12 18 23.4   11.3 10.0     ~ 1284 1
19 MCG-01-26-030 H2G 10 11 00.5 -04 41 30 12.48 12.13 11.93 11.78   ~ 789 2
20 NAME SDG G 18 55 19.0 -30 32 43   4.5 3.6     ~ 2438 2
21 NAME Sgr dIG G 19 29 59.0 -17 40 41   15.5 13.6     ~ 323 1
22 NGC 6822 G 19 44 56.199 -14 47 51.29   18 8.1     ~ 1661 0
23 M 15 GlC 21 29 58.33 +12 10 01.2           ~ 3274 0
24 Z 431-72 G 23 28 35.2 +14 44 35 13.85 13.16 12.52     ~ 499 1
25 NAME Peg dSph GiG 23 51 46.3 +24 34 57   14.5 13.2     ~ 250 2
26 NAME Local Group GrG ~ ~           ~ 9325 0

To bookmark this query, right click on this link: simbad:objects in 2019ApJ...877...49G and select 'bookmark this link' or equivalent in the popup menu