DOI QR코드

DOI QR Code

NEW SPECTROSCOPIC METHODS FOR THE SIMULTANEOUS ESTIMATION OF FUNDAMENTAL ATMOSPHERIC PARAMETERS USING THE LINE DEPTH RATIOUS

  • Kim, Chul-Hee (Division of Science Education, Institute of Fusion Science, Chonbuk National University) ;
  • Moon, B.K. (Division of Science Education, Institute of Fusion Science, Chonbuk National University) ;
  • Lee, I.H. (Division of Science Education, Institute of Fusion Science, Chonbuk National University)
  • 투고 : 2012.01.05
  • 심사 : 2012.02.23
  • 발행 : 2012.04.30

초록

New methods are developed to estimate the effective temperature (Te), surface gravity (log g), and metallicity ([A/H]) simultaneously with the spectral line depth ratios. Using the model atmosphere grids, depth values are calculated for the wavelength range of $4000{\AA}-5600{\AA}$ for various temperatures, gravities, and metallicities. All possible different combinations of line depth ratios for different pairs of ratios are investigated. A graphical 3D figure is produced with X, Y, and Z axes corresponding to Te, log g, and [A/H], respectively. By reading a cross point of two curves plotted by a connection of three parameters obtained from spectral line depth ratio pairs on each of the three projected planes, Te, log g, and [A/H] are determined simultaneously. In addition, an analytical method is devised based on the similar algorithm developed for the graphical method. Our methods were applied to estimate the fundamental atmospheric parameters of the Sun and Arcturus.

키워드

참고문헌

  1. Biemont, J., Palmeri, P., & Quinet, P. 2002, Database of Rare Earths At Mons University
  2. Fuhr, R., & Wiese, W. L. 2006, New Critical Compilations of Atomic Transition Probabilities for Neutral and Singly Ionized Carbon, Nitrogen, and Iron, J. Phys. Chem. Ref. Data, 35, 1669 https://doi.org/10.1063/1.2218876
  3. Gray, D. F. 1989, The Rotational Break for G Giants, ApJ, 347, 1021 https://doi.org/10.1086/168192
  4. Hinkle, K. et al. 2000, Visible and Near Infrared Atlas of the Arcturus Spectrum, Astron. Soc. of the Pacific
  5. Hirata, R., & Horaguchi, T. 1995, Atomic Spectral Line List, SIMBAD Catalog VI/69
  6. Kim, C. 2006, Spectral Line-Depth Ratio as a Precise Ef- fective Temperature and Surface Gravity Indicator for Warm Stars, J. Korean Astron. Soc, 39, 125 https://doi.org/10.5303/JKAS.2006.39.4.125
  7. Kim, C., & Moon, B.-K. 2011, A Method for the Simulta- neous Estimation of Atmospheric Parameters Using the Photometric Indices in the uvby Color System, AJ, 141, 118 https://doi.org/10.1088/0004-6256/141/4/118
  8. Kovtyukh, V. V., & Gorlova, N. L. 2000, Precise Tempera- tures of Classical Cepheids and Yellow Supergiants from Line-Depth Ratios, A&A, 358, 587
  9. Kurucz, R. L. 1993, CDROMs No. 1-18 (Cambridge, MA, Smithsonian Astrophys. Obs.)
  10. Kurucz, R. L. 1995, CDROM No. 23 (Cambridge, MA, Smithsonian Astrophys. Obs.)
  11. Morton, D. C. 2000, Atomic Data for Resonance Absorption Lines. II.Wavelengths Longward of the Lyman Limit for Heavy Elements, ApJS, 130, 403 https://doi.org/10.1086/317349
  12. Piskunov, N., Kupka, F., Ryabchikova, T., Weiss, W., & Jeffery, C. 1995, VALD: The Vienna Atomic Line Data Base, A&AS, 112, 525
  13. Ramirez, I., & Allende Prieto, C. 2011, Fundamental Pa- rameters and Chemical Composition of Arcturus, ApJ, 743, 135 https://doi.org/10.1088/0004-637X/743/2/135

피인용 문헌

  1. A method for the simultaneous estimation of the fundamental atmospheric parameters using the photometric indices in the BVRI and JHK color systems vol.351, pp.1, 2014, https://doi.org/10.1007/s10509-013-1700-2
  2. A SPECTROSCOPIC ANALYSIS OF THE K0 III BINARYϵCYGNI vol.810, pp.2, 2015, https://doi.org/10.1088/0004-637X/810/2/117
  3. A Spectroscopic Analysis of the Hyades Cool Giants vol.157, pp.3, 2019, https://doi.org/10.3847/1538-3881/aafc26