Hostname: page-component-cd9895bd7-dk4vv Total loading time: 0 Render date: 2024-12-18T23:02:13.116Z Has data issue: false hasContentIssue false
  • English
  • Français

The evolution of the oxygen abundance radial gradient in the Milky Way Galaxy disk

Published online by Cambridge University Press:  08 August 2017

Mercedes Mollá ,
Oscar Cavichia Open the ORCID record for Oscar Cavichia [Opens in a new window] ,
Roberto D. D. Costa ,
Walter J. Maciel ,
Brad Gibson Open the ORCID record for Brad Gibson [Opens in a new window]  and
Angeles I Díaz
Mercedes Mollá
Affiliation:
CIEMAT, Avda. Complutense 40, 28040 Madrid, Spain email: [email protected]
Oscar Cavichia
Affiliation:
Instituto de Física e Química, Universidade Federal de Itajubá, Av. BPS, 1303, 37500-903, Itajubá-MG, Brazil
Roberto D. D. Costa
Affiliation:
Instituto de Astronomia, Geofisica e Ciências Atmosféricas, Universidade de Sâo Paulo, 05508-900, Sâo Paulo-SP, Brazil
Walter J. Maciel
Affiliation:
Instituto de Astronomia, Geofisica e Ciências Atmosféricas, Universidade de Sâo Paulo, 05508-900, Sâo Paulo-SP, Brazil
Brad Gibson
Affiliation:
E.A Milne Centre for Astrophysics, University of Hull, HU6 7RX, United Kingdom
Angeles I Díaz
Affiliation:
Universidad Autónoma de Madrid, 28049, Madrid, Spain Astro-UAM, Unidad Asociada CSIC, Universidad Autónoma de Madrid,28049, Madrid, Spain
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We review the state of our chemical evolution models for spiral and low mass galaxies. We analyze the consequences of using different stellar yields, infall rate laws and star formation prescriptions in the time/redshift evolution of the radial distributions of abundances, and other quantities as star formation rate or gas densities, in the Milky Way Galaxy; In particular we will study the evolution of the oxygen abundance radial gradient analyzing its relation with the ratio SFR/infall. We also compare the results with our old chemical evolution models, cosmological simulations and with the existing data, mainly with the planetary nebulae abundances.

Keywords

galaxies: evolutiongalaxies: formationgalaxies: spiralgalaxies: abundances, Galaxy: abundances
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S323: Planetary Nebulae: Multi-Wavelength Probes of Stellar and Galactic Evolution , October 2016 , pp. 245 - 253
Copyright
Copyright © International Astronomical Union 2017 

References

Anders, F., Chiappini, C., Minchev, I., et al. 2016, A&A, submitted (arXiv:1608.04951)Google Scholar
Bergemann, M., et al., 2014, A&A, 565, A89 Google Scholar
Casagrande, L., Schönrich, R., Asplund, M., Cassisi, S., et al., 2011, A&A, 530, A138 Google Scholar
Cavichia, O., Costa, R. D. D., & Maciel, W. J., 2011, RMxAA, 47, 49 Google Scholar
Chen, L., Hou, J. L., & Wang, J. J., 2003, AJ, 125, 1397 CrossRefGoogle Scholar
Chiappini, C., Matteucci, F., & Gratton, R., 1997, ApJ, 477, 765 Google Scholar
Chieffi, A. & Limongi, M., 2004, ApJ, 608, 405 Google Scholar
Cresci, G., Mannucci, F., Maiolino, R., et al. 2010, Nature, 467, 811 (C10)Google Scholar
Costa, R. D. D., Cavichia, O., & Maciel, W. J., 2013, IAUS, 289, 375 Google Scholar
Cunha, K., Frinchaboy, P. M., Souto, D., et al. 2016, Astronomische Nachrichten, 337, 922 Google Scholar
Diaz, A. I. & Tosi, M., 1984, MNRAS, 208, 365 Google Scholar
Ferrini, F., Molla, M., Pardi, M. C., & Diaz, A. I., 1994, ApJ, 427, 745 CrossRefGoogle Scholar
Friel, E. D., Janes, K. A., Tavarez, M., Scott, J., Katsanis, R., et al., 2002, AJ, 124, 2693 CrossRefGoogle Scholar
Frinchaboy, P. M., et al., 2013, ApJ, 777, L1 Google Scholar
Gavilán, M., Buell, J. F., & Mollá, M., 2005, A&A, 432, 861 Google Scholar
Gavilán, M., Mollá, M., & Buell, J. F., 2006, A&A, 450, 509 Google Scholar
Gibson, B. K., Pilkington, K., Brook, C. B., Stinson, G. S., & Bailin, J. 2013, A&A, 554, A47 (G13)Google Scholar
Henry, R. B. C. & Worthey, G., 1999, PASP, 111, 919 CrossRefGoogle Scholar
Henry, R. B. C., Kwitter, K. B., Jaskot, A. E., et al. 2010, ApJ, 724, 748 (H10)Google Scholar
Hou, J. L., Prantzos, N., & Boissier, S., 2000, A&A, 362, 921 Google Scholar
Iwamoto, K., Brachwitz, F., Nomoto, K., et al. 1999, ApJS, 125, 439 Google Scholar
Jones, T., Ellis, R. S., Richard, J., & Jullo, E. 2013, ApJ, 765, 48 (J13)Google Scholar
Kroupa, P., 2002, Sci, 295, 82 Google Scholar
Lacey, C. G. & Fall, S. M., 1983, MNRAS, 204, 791 Google Scholar
Lacey, C. G. & Fall, S. M., 1985, ApJ, 290, 154 Google Scholar
Limongi, M. & Chieffi, A., 2003, ApJ, 592, 404 Google Scholar
Maciel, W. J., Costa, R. D. D., & Uchida, M. M. M., 2003, A&A, 397, 667 Google Scholar
Maciel, W. J. & Costa, R. D. D. 2013, RMxA&Ap, 49, 333 (M13)Google Scholar
Magrini, L., Sestito, P., Randich, S., & Galli, D., 2009, A&A, 494, 95 Google Scholar
Magrini, L., Coccato, L., Stanghellini, L., Casasola, V., & Galli, D. 2016, A&A, 588, A91 Google Scholar
Matteucci, F., & Francois, P., 1989, MNRAS, 239, 885 CrossRefGoogle Scholar
McCall, M. L., Rybski, P. M., & Shields, G. A. 1985, ApJS, 57, 1 Google Scholar
Mollá, M., Díaz, A. I., & Tosi, M., 1990, in Chemical and dynamical evolution of Galaxies, eds. Ferrini, F., Franco, J., & Matteucci, F., ETS Editrice (PISA), 577Google Scholar
Mollá, M., Ferrini, F., & Diaz, A. I., 1997, ApJ, 475, 519 Google Scholar
Mollá, M. & Díaz, A. I. 2005, MNRAS, 358, 521 (MD05)Google Scholar
Mollá, M., Cavichia, O., Gavilán, M., & Gibson, B. K., 2015, MNRAS, 451, 3693 Google Scholar
Mollá, M., Díaz, A. I., Gibson, B. K., et al., 2016, MNRAS, 462, 1329 Google Scholar
Mollá, M., Ascasibar, Y., Díaz, A. I., & Gibson, B. K., 2017, MNRAS, submitted (M16)Google Scholar
Nordström, B., et al., 2004, A&A, 418, 989 Google Scholar
Pilkington, K., Few, C. G., Gibson, B. K., et al. 2012, A&A, 540, A56 Google Scholar
Portinari, L. & Chiosi, C., 2000, A&A, 355, 929 Google Scholar
Prantzos, N. & Aubert, O., 1995, A&A, 302, 69 Google Scholar
Queyrel, J., Contini, T., Kissler-Patig, M., et al. 2012, A&A, 539, A93 (Q12)Google Scholar
Rupke, D. S. N., Kewley, L. J., & Chien, L.-H. 2010, ApJ, 723, 1255 (R10)Google Scholar
Salucci, P., Lapi, A., Tonini, C., Gentile, G., et al., 2007, MNRAS, 378, 41 Google Scholar
Sánchez, S. F., Rosales-Ortega, F. F., Iglesias-Páramo, J., et al. 2014, A&A, 563, A49 (S14)Google Scholar
Shaver, P. A., McGee, R. X., Newton, L. M., Danks, A. C., et al. 1983, MNRAS, 204, 53 Google Scholar
Stanghellini, L. & Haywood, M. 2010, ApJ, 714, 1096 (S10)CrossRefGoogle Scholar
Tosi, M. & Díaz, A. I. 1985, MNRAS, 217, 571 Google Scholar
Xiang, M.-S., Liu, X.-W., Yuan, H.-B., et al. 2015, Research in Astronomy and Astrophysics, 15, 1209 Google Scholar
Yuan, T.-T., Kewley, L. J., Swinbank, A. M., et al.., 2011, ApJL, 732, L14 Google Scholar
Zaritsky, D., Kennicutt, R. C. Jr, & Huchra, J. P., 1994, ApJ, 420, 87 Google Scholar