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Grids J/A+AS/135/405 of stellar models. VIII. (Charbonnel+ 1999) ================================================================================ Grids of stellar models. VIII. From 0.4 to 1.0 M_Sun_ at Z=0.020 and Z=0.001, with the MHD equation of state Charbonnel C., Dappen W., Schaerer D., Bernasconi P.A., Maeder A., Meynet G., Mowlavi N. <Astron. Astrophys. Suppl. Ser. 135, 405 (1999)> =1999A&AS..135..405C (SIMBAD/NED BibCode) ================================================================================ ADC_Keywords: Models, evolutionary ; Mass loss ; HR diagrams Keywords: stars: evolution - stars: Hertzsprung-Russel diagram stars: interiors - stars: low-mass Abstract: We present stellar evolutionary models covering the mass range from 0.4 to 1M_{sun}_ calculated for metallicities Z=0.020 and 0.001 with the MHD equation of state (Hummer & Mihalas, 1988ApJ...331..794H, Mihalas et al., 1988ApJ...331..815M, Daeppen et al., 1988ApJ...332..261D). A parallel calculation using the OPAL (Rogers et al., 1996ApJ...456..902R) equation of state has been made to demonstrate the adequacy of the MHD equation of state in the range of 1.0 to 0.8M_{sun}_ (the lower end of the OPAL tables). Below, down to 0.4M_{sun}_, we have justified the use of the MHD equation of state by theoretical arguments and the findings of Chabrier & Baraffe (1997A&A...327.1039C). We use the radiative opacities by Iglesias & Rogers (1996ApJ...464..943I), completed with the atomic and molecular opacities by Alexander & Fergusson (1994ApJ...437..879A). We follow the evolution from the Hayashi fully convective configuration up to the redgiant tip for the most massive stars, and up to an age of 20Gyr for the less massive ones. We compare our solar-metallicity models with recent models computed by other groups and with observations. File Summary: -------------------------------------------------------------------------------FileName Lrecl Records Explanations -------------------------------------------------------------------------------ReadMe 80 . This file table1.dat 258 2 0.4M, Z=0.001, Y=0.243, without overshooting table2.dat 258 3 0.5M, Z=0.001, Y=0.243, without overshooting table3.dat 258 6 0.6M, Z=0.001, Y=0.243, without overshooting table4.dat 258 11 0.7M, Z=0.001, Y=0.243, without overshooting table5.dat 258 51 0.8M, Z=0.001, Y=0.243, without overshooting table6.dat 258 51 0.9M, Z=0.001, Y=0.243, without overshooting table7.dat 256 51 1.0M, Z=0.001, Y=0.243, without overshooting table8.dat 256 3 0.4M, Z=0.020, Y=0.300, without overshooting table9.dat 256 4 0.5M, Z=0.020, Y=0.300, without overshooting table10.dat 256 5 0.6M, Z=0.020, Y=0.300, without overshooting table11.dat 256 11 0.7M, Z=0.020, Y=0.300, without overshooting table12.dat 256 14 0.8M, Z=0.020, Y=0.300, without overshooting table13.dat 256 51 0.9M, Z=0.020, Y=0.300, without overshooting table14.dat 256 51 1.0M, Z=0.020, Y=0.300, without overshooting table15.dat 256 3 0.4M, Z=0.020, Y=0.280, without overshooting table16.dat 256 4 0.5M, Z=0.020, Y=0.280, without overshooting table17.dat 256 5 0.6M, Z=0.020, Y=0.280, without overshooting table18.dat 256 7 0.7M, Z=0.020, Y=0.280, without overshooting table19.dat 256 14 0.8M, Z=0.020, Y=0.280, without overshooting table20.dat 256 51 0.9M, Z=0.020, Y=0.280, overshooting without table21.dat 256 51 1.0M, Z=0.020, Y=0.280, without overshooting -------------------------------------------------------------------------------See also: J/A+AS/96/269 : Paper J/A+AS/98/523 : Paper J/A+AS/101/415 : Paper J/A+AS/102/339 : Paper J/A+AS/103/97 : Paper 0.040 (Meynet+ 1994) J/A+AS/115/339 : Paper J/A+AS/128/471 : Paper I. II. III. IV. V. 0.8 to 120 M_{sun}_, Z=0.020 0.8 to 120 M_{sun}_, Z=0.008 0.8 to 120 M_{sun}_, Z=0.004 0.8 to 120 M_{sun}_, Z=0.040 12 to 120 M_{sun}_, Z=0.001, (Schaller+, 1992) (Schaerer+ 1993) (Charbonnel+ 1993) (Schaerer+, 1993) 0.004, 0.008, 0.020 VI. HB abd AGB, Z=0.020, 0.001 (Charbonnel+, 1996) VII. 0.8 to 60M_{sun}_, Z=0.10 (Mowlavi+ 1998) Byte-by-byte Description of file: table1.dat, table2.dat, table3.dat, table4.dat Byte-by-byte Description of file: table5.dat, table6.dat, table7.dat, table8.dat Byte-by-byte Description of file: table9.dat, table10.dat, table11.dat Byte-by-byte Description of file: table12.dat, table13.dat, table14.dat Byte-by-byte Description of file: table15.dat, table16.dat, table17.dat Byte-by-byte Description of file: table18.dat, table19.dat, table20.dat Byte-by-byte Description of file: table21.dat -------------------------------------------------------------------------------Bytes Format Units Label Explanations -------------------------------------------------------------------------------1- 2 I2 --Npoint Number of selected point 4- 17 E14.7 yr Age Age 18- 25 F8.4 solMass Mass Actual mass 27- 32 F6.3 [solLum] log(L) log(luminosity) 34- 38 F5.3 [K] log(Teff) log(effective temperature) 40- 47 F8.6 --Hs H surface abundance (mass fraction) 49- 56 F8.6 --Hes He surface abundance (mass fraction) 58- 65 F8.6 --12Cs 12C surface abundance (mass fraction) 67- 74 F8.6 --13Cs 13C surface abundance (mass fraction) 76- 83 F8.6 --14Ns 14N surface abundance (mass fraction) 85- 92 F8.6 --16Os 16O surface abundance (mass fraction) 94-101 F8.6 --17Os 17O surface abundance (mass fraction) 103-110 F8.6 --18Os 18O surface abundance (mass fraction) 112-119 F8.6 --20Nes 20Ne surface abundance (mass fraction) 121-128 F8.6 --22Nes 22Ne surface abundance (mass fraction) 130-136 F7.5 --QCC Core mass fraction 143-149 F7.3 solMass/yr Mdot log(mass loss rate) 152-156 F5.3 [g/cm3] rhoc log(central density) 158-162 F5.3 [K] log(Tc) log(central temperature) 164-171 F8.6 --Hc H central abundance (mass fraction) 173-180 F8.6 --Hec He central abundance (mass fraction) 182-189 F8.6 --12Cc 12C central abundance (mass fraction) 191-198 F8.6 --13Cc 13C central abundance (mass fraction) 200-207 F8.6 --14Nc 14N central abundance (mass fraction) 209-216 F8.6 --16Oc 16O central abundance (mass fraction) 218-225 F8.6 --17Oc 17O central abundance (mass fraction) 227-234 F8.6 --18Oc 18O central abundance (mass fraction) 236-243 F8.6 --20Nec 20Ne central abundance (mass fraction) 245-252 F8.6 --22Nec 22Ne central abundance (mass fraction) -------------------------------------------------------------------------------History: Pre-main sequence tracks can be asked to Corinne.Charbonnel@obs-mip.fr Acknowledgements: Corinne Charbonnel <corinne.charbonnel@ast.obs-mip.fr> ================================================================================ (End) Patricia Bauer [CDS] 14-Dec-1998
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EDHD 426. Section 0401 Cognition and Motivation in Reading: Reading in Content Areas I University of Maryland, College Park Thursday 4:15 to 7:00 Benjamin Building Room 3315 Fall 2004 Instructor: Ana Taboada. E-mail: ataboada@umd.edu Office Phone: 3...
Maryland >> HIST >> 426 (Fall, 2008)
Fall 2007 EDCI 426: Materials and Resources in Social Studies Instructor: Lisa Eaker Office: 2304 Benjamin Building Office Hours: Wednesday 11:30-3:30 and by appointment. Email: lisae@umd.edu EDU 2212 Phone number: (202) 680-9628 Class Meetings: Wed...
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news and views that led to the stunning realization that all photosystems are basically alike and must have the same evolutionary origin. A more detailed comparison of the two photosystems should soon be possible: we now have Jordan et al.s high-reso...
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NRAC Publication No. 106-2008 University of Maryland, 2113 Animal Science Building College Park, Maryland 20742-2317 Telephone: 301-405-6085, FAX: 301-314-9412 E-mail: nrac@umd.edu Web: http:/www.nrac.umd.edu Fish Health Inspections: What They Are ...
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GEOG 140 Estuaries 1. Importance of Estuaries estuaries are produced when rivers meet the sea. -because of this, due to source of nutrients, estuaries are very productive -the amount of biomass in estuaries is only matched to a certain degree by coas...
Maryland >> HLTH >> 140 (Fall, 2008)
140: Matters of Life and Death 25 Famine (3): Life-boat Ethics 1 Judgment day (Pascal in Singer 1986.) The first two-thirds of Pascals paper depend upon rejecting the active/passive, and/or justice/charity, distinction. (Failing the save is the sam...
Maryland >> HLTH >> 140 (Fall, 2008)
140: Matters of Life and Death 17 Animals (1): Utilitarianism & Animal Suffering 1 Overview: the threat to common-sense The basic point at issue is: in virtue of what properties does a being attain moral standing? The common-sense view is that anim...
Maryland >> HLTH >> 150 (Fall, 2008)
ABSTRACT Title of Thesis: EFFECT OF ACID ADAPTATION ON THE THERMAL INACTIVATION OF LISTERIA MONOCYTOGENES IN HEATING MENSTRUA HAVING VARIOUS COMBINATIONS OF PH AND WATER ACTIVITIES Sharon G. Edelson-Mammel, Master of Science, 2003 Thesis Directed...
Maryland >> HLTH >> 150 (Fall, 2008)
Microbiology (2004), 150, 12911299 DOI 10.1099/mic.0.26727-0 Enhanced motility of a Proteus mirabilis strain expressing hybrid FlaAB agella Jim Manos, Elena Artimovich and Robert Belas Correspondence Robert Belas belas@umbi.umd.edu Center of Marin...
Maryland >> HLTH >> 230 (Fall, 2008)
EDHD 230: Human Development and Societal Institutions Spring, 2005, Section 0101 Tuesday and Thursday 9:30am 10:45am in Cole 3110 Instructor: Bella M. Guner Office: 4315 Benjamin Building University of Maryland, College Park Department of Human Deve...
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