Absolute Magnitudes of Seismic Red Clumps in the Kepler Field and SAGA: the age dependency of the distance scale

Preprint English OPEN
Chen, Y. Q. ; Casagrande, L. ; Zhao, G. ; Bovy, J. ; Aguirre, V. Silva ; Zhao, J. K. ; Jia, Y. P. (2017)
  • Related identifiers: doi: 10.3847/1538-4357/aa6d0f
  • Subject: Astrophysics - Solar and Stellar Astrophysics | Astrophysics - Astrophysics of Galaxies
    arxiv: Astrophysics::Galaxy Astrophysics | Astrophysics::Cosmology and Extragalactic Astrophysics | Astrophysics::Earth and Planetary Astrophysics | Astrophysics::Solar and Stellar Astrophysics

Red clump stars are fundamental distance indicators in astrophysics, although theoretical stellar models predict a dependence of absolute magnitudes with ages. This effect is particularly strong below 2 Gyr, but even above this limit a mild age dependence is still expected. We use seismically identified red clump stars in the Kepler field for which we have reliable distances, masses and ages from the SAGA survey to first explore this effect. By excluding red clump stars with masses larger than 1.6 Msun (corresponding to ages younger than 2 Gyr), we derive robust calibrations linking intrinsic colors to absolute magnitudes in the following photometric systems: Str\"omgren $by$, Johnson $BV$, Sloan $griz$, 2MASS $JHK_s$ and WISE $W1W2W3$. With the precision achieved we also detect a slope of absolute magnitudes 0.020(0.003) mag per Gyrin the infrared, implying that distance calibrations of clump stars can be off by up to 0.2 mag in the infrared (over the range from 2 Gyr to 12 Gyr) if their ages are unknown. Even larger uncertainties affect optical bands, because of the stronger interdependency of absolute magnitudes on colors and age. Our distance calibrations are ultimately based on asteroseismology, and we show how the distance scale can be used to test the accuracy of seismic scaling relations. Within the uncertainties our calibrations are in agreement with those built upon local red clump with Hipparcos} parallaxes, although we find a tension which if confirmed would imply that scaling relations overestimate radii of red clump stars by 2(+-20%. Data-releases post Gaia DR1 will provide an important testbed for our results.
  • References (17)
    17 references, page 1 of 2

    Auvergne M et al., 2009, A&A, 506, 411 Basu S. et al., 2011, ApJ, 729, L10 Bedding, T.R. et al., 2011, Natur, 471, 608 Bilir, S., Ak, T., Ak, S., Yontan, T., Bostanc, Z.F., 2013a, NewA, 23, 88 Bilir, S., Onal, O., Karaali, S., Cabrera-Lavers, A., Cakmak, H., 2013b. Ap&SS, 344, 417 Brogaard, K., Jessen-Hansen, J., Handberg, R., et al. 2016, Astronomische Nachrichten, 337, 793

    Brown, T. M., Latham, D. W., Everett, M. E., & Esquerdo, G. A. 2011, AJ, 142, 112 Calamida A., Bono G., Lagioia E.P. et al. 2014, A&A, 565, 8 Girardi L., Groenewegen M. A. T., Weiss A., Salaris M., 1998, MNRAS, 301, 149 Girardi L., Mermilliod J.-C., Carraro G., 2000, A&A, 354, 892 Girardi L. & Salaris M., 2001, MNRAS, 323, 109 Groenewegen, M.A.T.: 2008, A&A, 488, 25 Grocholski, A.J., Sarajedini, A., 2002, AJ, 123, 1603 Hekker S. et al., 2011a, A&A, 530, A100 Henden, A. A., Welch, D. L., Terrell, D., & Levine, S. E. 2009, American Astronomical Society Meeting Abstracts #214, 214, #407.02

    Hesser, J.E. & Hartwick, F.D.A, 1977, ApJS, 33, 361 Hogg, D.W., Bovy, J., & Lang D. astro-ph/1008.4686v1 Huber D. et al., 2010, ApJ, 723, 1607 Huber, D., Ireland, M. J., Bedding, T. R., et al. 2012, ApJ, 760, 32 Huber, D., Silva Aguirre, V., Matthews, J. M., et al. 2014, ApJS, 211, 2 Miglio, A., Chiappini, C., Morel, T., et al. 2013, European Physical Journal Web of Conferences, 43, 03004

    Montalb´an, J et al. 2010, ApJL 721, 182

    Montalb´an, J et al. 2013, ApJ 766, 118

    Paczyn´ski B. & Stanek K. Z., 1998, ApJ, 494, 219

    Pinsonneault, M. H., An, D., Molenda- Z˙akowicz, J., et al. 2012, ApJS, 199, 30 Rodrigues, T. S., Girardi, L., Miglio, A., et al. 2014, MNRAS, 445, 2758 Silva Aguirre, V., Casagrande, L., Basu, S., et al. 2012, ApJ, 757, 99

    Skrutskie M. F. et al., 2006, AJ, 131, 1163

    Stanek, K. Z. & Garnavich, P. M., 1998, ApJ, 503, 131

    Stello, D., Chaplin, W.J., Basu, S., Elsworth, Y., & Bedding, T. R. 2009, MNRAS, 400, L80 Stello, D., Huber, D., Bedding, T. R., et al. 2013, ApJ, 765, L41

  • Metrics
    No metrics available
Share - Bookmark