ULIRG NaD fits
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(km/s) |
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two independent pairs; "A" fixed to have CO velocity = 31688 km/s. | 424 +/- 37 | 416 +/- 43 | 1.49 +/- 0.08 |
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31076 +/- |
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same as in fig2a, but with HeI line also fixed to have CO velocity. | 557 +/- 147 | 829 +/- 515 | 0.9 +/- 1.2 |
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same as in fig2b, but "A" FWHM fixed at 388 km/s. This is a bad fit. | NA | 1007 +/- 9 | negative ?? | 8.60 +/- 0.07 |
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same as in fig2c, but with red "A" EQW fixed at 0.22371 angstroms. | NA | 927 +/- 22 | NA | 7.07 +/- 0.08 |
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same as in fig2a, except there is no HeI emission line. | 581 +/- 78 | 698 +/- 83 | 1.16 +/- 0.27 | 4.6 +/- 0.6 |
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two independent pairs; "A" fixed to have CO velocity = 19330 km/s. | 794 +/- 89 | 750 +/- 150 | 1.1 +/- 0.1 | 1.6 +/- 0.2 |
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same as in fig2a, but "A" FWHM fixed at 388 km/s. | NA | 379 +/- 45 | 0.87 +/- 0.03 | 1.9 +/- 0.2 |
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same as in fig2b, but with red "A" EQW fixed at 0.17897 angstroms. | NA | 1034 +/- 45 | NA | 3.4 +/- 0.1 |
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same as in fig2a, except there is no HeI emission line. | 753 +/- 40 | 315 +/- 34 | 1.11 +/- 0.05 | 0.95 +/- 0.08 |
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iras2336_fig2e.ps | same as in fig2c, except there is no HeI emission line. | NA | 714 +/- 30 | NA | 2.65 +/- 0.09 |
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iras2336.plt2e |
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one FWHM for both pairs. Continuum slope is free. | 493 +/- 12 | NA | 0.37 +/- 0.01 | 2.10 +/- 0.07 |
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two independent pairs. | 478 +/- 25 | 542 +/- 85 | 0.35 +/- 0.06 | 2.2 +/- 0.6 |
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two independent pairs; "A" fixed to have CO velocity = 29173 km/s. | 451 +/- 65 | 512 +/- 72 | 0.33 +/- 0.03 | 2.2 +/- 0.7 |
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same as in fig3, but with red "A" EQW fixed at 0.111857 angstroms. | 534 +/- 334 | 730 +/- 80 | NA | 3.1 +/- 0.7 |
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same as in fig4, but "A" FWHM fixed at 388 km/s. | NA | 701 +/- 63 | NA | 2.7 +/- 0.3 |
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same as in fig3, except there is no HeI emission line. | 541 +/- 51 | 255 +/- 23 | 0.46 +/- 0.04 | 0.48 +/- 0.06 |
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two independent pairs; "A" fixed to have CO velocity = 40044 km/s. | 504 +/- 28 | 399 +/- 39 | 1.06 +/- 0.09 | 2.6 +/- 0.6 |
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same as in fig2a, but "A" FWHM fixed at 388 km/s. | NA | 403 +/- 70 | 0.90 +/- 0.09 | 2.6 +/- 1.2 |
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same as in fig2b, but with red "A" EQW fixed at 0.09284 angstroms. | NA | 919 +/- 59 | NA | 3.9 +/- 0.5 |
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same as in fig2a, except there is no HeI emission line. | 530 +/- 36 | 258 +/- 37 | 1.08 +/- 0.08 | 0.5 +/- 0.1 |
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two independent pairs; "A" fixed to have CO velocity = 27674 km/s. | 265 +/- 18 | 778 +/- 73 | 1.51 +/- 0.09 | 2.4 +/- 0.4 |
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same as in fig2a, but "A" FWHM fixed at 388 km/s. This is a bad fit. | NA | 1561 +/- 151 | 1.94 +/- 0.09 | 3.4 +/- 0.5 |
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same as in fig2a ("A" FWHM free), but with red "A" EQW fixed at 0.04474 angstroms. | 535 +/- 930 | 424 +/- 26 | NA | 4.5 +/- 0.2 |
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same as in fig2b, but with red "A" EQW fixed at 0.04474 angstroms. "A" FWHM fixed at 388 km/s. | NA | 422 +/- 23 | NA | 4.5 +/- 0.2 | 27648 +/- |
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same as in fig2a, except there is no HeI emission line. | 172 +/- 42 | 509 +/- 29 | 0.7 +/- 0.2 | 3.9 +/- 0.5 |
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three absorption pairs; "A" fixed to have CO velocity = 27674 km/s. |
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two independent pairs; "A" fixed to have CO velocity = 25700 km/s | 282 +/- 60 | 545 +/- 104 | 0.24 +/- 0.08 | 3.0 +/- 0.5 |
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same as in fig2a, but "A" FWHM fixed at 388 km/s. | NA | 586 +/- 228 | 0.2 +/- 0.1 | 3.1 +/- 0.9 |
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same as in fig2b, but with red "A" EQW fixed at 0.14318 angstroms. | NA | 616 +/- 70 | NA | 3.2 +/- 0.3 |
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same as in fig2a, except there is no HeI emission line. | 345 +/- 60 | 382 +/- 26 | 0.36 +/- 0.06 | 2.2 +/- 0.1 |
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New fits for paper (these are all without HeI emission, which is un-physical for 0026, 1609, 1049, and maybe 1929)
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(km/s) |
(km/s) |
(km/s) |
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same as in fig2d, but "B" doublet ratio is free. The "A" doublet ratio is fixed at 1.98:1. There is no HeI emission line. |
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same as in fig2f, but the "A" doublet ratio is fixed at 1:1. |
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iras2336.plt2g |
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same as in fig6, but "B" doublet ratio is free. The "A" doublet ratio is fixed at 1.98:1. The continuum slope and intercept fixed at best-fit values from fig6. There is no HeI emission line. |
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iras0026.plt6a |
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same as in fig6, but "B" doublet ratio is free. The "A" doublet ratio is fixed at 1:1. The continuum slope and intercept fixed at best-fit values from fig6. There is no HeI emission line. |
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same as in fig2e, but "B" doublet ratio is free. The "A" doublet ratio is fixed at 1.98:1. There is no HeI emission line. |
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iras2008.plt2f |
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same as in fig2f, but the "A" doublet ratio is fixed at 1:1. |
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iras2008.plt2g |
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same as in fig2d, but "B" doublet ratio is free. The "A" doublet ratio is fixed at 1.98:1. There is no HeI emission line. (this fit did not converge) |
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red "B" not confidently detected |
iras1609.plt2e |
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same as in fig2e, but the "A" doublet ratio is fixed at 1:1. |
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iras1049_fig2f.ps | same as in fig2e, but "B" doublet ratio is free. The "A" doublet ratio is fixed at 1.98:1. There is no HeI emission line. |
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iras1049.plt2f |
iras1049_fig2g.ps | same as in fig2f, but the "A" doublet ratio is fixed at 1:1. |
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iras1049.plt2g |
iras1049_fig2h.ps | same as in fig2e, but "B" doublet ratio is fixed at 1:1. The "A" doublet ratio is fixed at 1.98:1. There is no HeI emission line. | 0.22 +/- | 27554 +/- 12 | 150 +/- 30 | 445 +/- 25 |
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iras1049.plt2h |
iras1049_fig2i.ps | same as in fig2h, but the "A" doublet ratio is fixed at 1:1 also. | 0.54 +/- | 27422 +/- 23 | 232 +/- 15 | 321 +/- 40 |
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iras1049.plt2i |
iras1929_fig2e.ps | same as in fig2d, but "B" doublet ratio is free. The "A" doublet ratio is fixed at 1.98:1. There is no HeI emission line. |
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iras1929_fig2f.ps | same as in fig2e, but the "A" doublet ratio is fixed at 1:1. |
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iras1929.plt2f |
Notes: "A" EQW frac = the sum of the blue and red stellar
component EQWs divided by the sum of the stellar and interstellar EQWs.
"B" vel = the recessional velocity of the interstellar doublet.
"B" doublet ratio = the EQW ratio of the blue and red lines of the interstellar
component (blue/red).