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A Carbon Star Survey in the Local Group galaxies

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A Carbon Star Survey in the Local Group galaxies. [email protected]. Roma, 4 Novembre 1868: the Beginning!. A Carbon Star Survey in the Local Group galaxies. CS as standard candles CS as tracers of low density halos & tidal tales CS as kinematical probes. Contents:. - PowerPoint PPT Presentation
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Page 2: A Carbon Star Survey  in the Local Group galaxies

Roma, 4 Novembre 1868: the Beginning!

Page 3: A Carbon Star Survey  in the Local Group galaxies

Contents:Contents:

[email protected] [email protected]

CS as standard candlesCS as standard candles

CS as tracers of low density halos & tidal talesCS as tracers of low density halos & tidal tales

CS as kinematical probes CS as kinematical probes

Page 4: A Carbon Star Survey  in the Local Group galaxies

Standard CandlesTheory

Evolutionary models of Evolutionary models of stellar systems suggest stellar systems suggest that <Mthat <Mbolbol> of CS does > of CS does not depend on the not depend on the metallicity.metallicity.(see e.g. Mouhcine&Lançon, (see e.g. Mouhcine&Lançon, 2003)2003)

Powerful standard candles:

brighter than Cepheids;

single epoch of observation;

reduced absorption (NIR);

brighter than the TRGB.

Page 5: A Carbon Star Survey  in the Local Group galaxies

Standard Candlesobservations

absolute magnitudes of CN stars span over 8mag !! (Knapp et al. 2000)

cool red-giant size ~10mas with spatial and temporal variation in surface brightness

hard to draw conclusions

Page 6: A Carbon Star Survey  in the Local Group galaxies

• Palmer & Wing (1982)• Cook & Aaronson (1989)• Richer et al. (V,I,CN,TiO)• B&D (R,I,CN,TiO)

Four Band Photometric System

Page 7: A Carbon Star Survey  in the Local Group galaxies

Standard Candlesresults from our ongoing survey

When CS are carefully When CS are carefully and homogeneously and homogeneously identifiedidentified(FBPS in our survey):(FBPS in our survey):

<M<MII> independent of > independent of [Fe/H][Fe/H] <M<MII> scatter for faint > scatter for faint galaxiesgalaxies

Page 8: A Carbon Star Survey  in the Local Group galaxies

Low-Density Environment Tracersresults from our ongoing survey

The case of NGC 6822 The case of NGC 6822 and its extended and its extended halo….halo….

Intermediate-age halo

First d

etection!

… … of old and of old and intermediate ageintermediate age stars. stars.

Page 9: A Carbon Star Survey  in the Local Group galaxies

Low-Density Environment Tracersresults from our ongoing survey

… … and the missing and the missing halo of NGC 3109…halo of NGC 3109…

exp. disk:exp. disk: 2.96± 0.14 arcmin2.96± 0.14 arcmin

minor minor axis:axis: 4-5 arcmin4-5 arcmin

Page 10: A Carbon Star Survey  in the Local Group galaxies

Low-Density Environment Tracersresults from our ongoing survey

… … the tidal debris the tidal debris around NGC 205.around NGC 205.

About 500 CS identified About 500 CS identified (2003, AJ June)(2003, AJ June)

Page 11: A Carbon Star Survey  in the Local Group galaxies

Low-Density Environment Tracersresults from our ongoing survey

… … the tidal debris the tidal debris around NGC 205.around NGC 205.

Extratidal stars NW of NGC 205Extratidal stars NW of NGC 205

Page 12: A Carbon Star Survey  in the Local Group galaxies

Kinematical Probesfollow-up of our survey

the stellar rotation the stellar rotation curve and the mass of curve and the mass of Andromeda galaxyAndromeda galaxy

900 CS identified 900 CS identified along the SW major axis along the SW major axis from 17 to 30 from 17 to 30 (2003 AJ, 125, (2003 AJ, 125, 1298)1298)

extention up to 40 kpc extention up to 40 kpc (TNG-QSO, July 03)(TNG-QSO, July 03)

Page 13: A Carbon Star Survey  in the Local Group galaxies

Kinematical Probesfollow-up of our survey

the stellar rotation the stellar rotation curve and the mass of curve and the mass of Andromeda galaxyAndromeda galaxy

900 CS identified 900 CS identified along the SW major axis along the SW major axis from 17 to 30 from 17 to 30 (2003 AJ, 125, (2003 AJ, 125, 1298)1298)

extention up to 40 kpc extention up to 40 kpc (TNG-QSO, July 03)(TNG-QSO, July 03)20 kpc = 8020 kpc = 80''

30 kpc = 13030 kpc = 130''40 kpc = 18040 kpc = 180''

Page 14: A Carbon Star Survey  in the Local Group galaxies

Kinematical Probesfollow-up of our survey

the stellar rotation the stellar rotation curve and the mass of curve and the mass of Andromeda galaxyAndromeda galaxy

beyond 30kpc only 2 beyond 30kpc only 2 GCs and none PNGCs and none PN this will provide the this will provide the largest lowerlargest lower estimate of estimate of the mass of M 31the mass of M 31

Gemini N Gemini N

TN

G

TN

G

Page 15: A Carbon Star Survey  in the Local Group galaxies

Kinematical Probesfollow-up of our survey

… … the monstrous MegaPrimethe monstrous MegaPrime

Page 16: A Carbon Star Survey  in the Local Group galaxies

Kinematical Probesfollow-up of our survey

… … the monstrous MegaPrimethe monstrous MegaPrime

CS: e.g. Margon et al. 2002CS: e.g. Margon et al. 2002

Page 17: A Carbon Star Survey  in the Local Group galaxies

GalaxyGalaxy NNCSCS StatusStatus

IC 1613IC 1613 195195 publishedpublished

PagasusPagasus 4040 publishedpublished

DDO 210DDO 210 33 publishedpublished

SagDIrrSagDIrr 1616 publishedpublished

Leo ILeo I 1313 publishedpublished

NGC 6822NGC 6822 904904 publishedpublished

M 31 M 31 (part.)(part.) 945945 publishedpublished

NGC 205NGC 205 532532 publishedpublished

NGC 3109NGC 3109 326326 submittedsubmitted

NGC 147NGC 147 288288 in in preparationpreparation

NGC 185NGC 185 +100+100 in in preparationpreparation

IC 10IC 10 +100+10000

just donejust done

WLMWLM ------ data data acquiredacquired

CS survey in the Local CS survey in the Local GroupGroup

IC 10IC 10


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