A Method for Deriving Accurate Gas‐Phase Abundances for the Multiphase Interstellar Galactic Halo

J. Christopher Howk; Kenneth R. Sembach; Blair D. Savage

doi:10.1086/497352

journal article Jan 20, 2006

A Method for Deriving Accurate Gas‐Phase Abundances for the Multiphase Interstellar Galactic Halo

J. Christopher Howk Kenneth R. Sembach Blair D. Savage

The Astrophysical Journal Vol. 637 No. 1 pp. 333-341 · American Astronomical Society

View at Publisher Save 10.1086/497352

Topics

No keywords indexed for this article. Browse by subject →

References

49

[1]

Andre, M., et al. 2003, ApJ, 591, 1000 10.1086/375530

[2]

Arabadjis, J. S. & Bregman, J. N. 1999, ApJ, 510, 806 10.1086/306616

[3]

Asplund, M., Grevesse, N. & Sauval, A. J. 2005, in ASP Conf. Ser. 336, Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis, ed. F. N. Bash & T. G. Barnes (San Francisco: ASP), 25

[4]

Bohlin, R. C., Savage, B. D. & Drake, J. F. 1978, ApJ, 224, 132 10.1086/156357

[5]

Danly, L., Lockman, F. J., Meade, M. R. & Savage, B. D. 1992, ApJS, 81, 125 10.1086/191689

[6]

Diplas, A. & Savage, B. D. 1994, ApJS, 93, 211 10.1086/192052

[7]

Dixon, W. V., Davidsen, A. F. & Ferguson, H. C. 1994, AJ, 107, 1388 10.1086/116952

[8]

Domgorgen, H. & Mathis, J. S. 1994, ApJ, 428, 647 10.1086/174275

[9]

Fang, T., Sembach, K. R. & Canizares, C. R. 2003, ApJ, 586, L49 10.1086/374680

[10]

Freire, P. C., Kramer, M., Lyne, A. G., Camilo, F., Manchester, R. N. & D’Amico, N. 2001, ApJ, 557, L105 10.1086/323248

[11]

Futamoto, K., Mitsuda, K., Takei, Y., Fujimoto, R. & Yamasaki, N. Y. 2004, ApJ, 605, 793 10.1086/381087

[12]

Standard Solar Composition

N. Grevesse, A.J. Sauval

Space Science Reviews 10.1023/a:1005161325181

[13]

Haffner, L. M., Reynolds, R. J. & Tufte, S. L. 1999, ApJ, 523, 223 10.1086/307734

[14]

Hartmann, D. & Burton, W. B. 1997, Atlas of Galactic Neutral Hydrogen (Cambridge: Cambridge Univ. Press)

[15]

Howk, J. C. & Savage, B. D. 1999, ApJ, 517, 746 10.1086/307211

[16]

Howk, J. C., Savage, B. D. & Fabian, D. 1999, ApJ, 525, 253 10.1086/307888

[17]

Howk, J. C. & Sembach, K. R. 1999, ApJ, 523, L141 10.1086/312284

[18]

Howk, J. C., Sembach, K. R. & Savage, B. D. 2003, ApJ, 586, 249 (Paper I) 10.1086/346262

[19]

Jenkins, E. B. 1971, ApJ, 169, 25 10.1086/151114

[20]

Lockman, F. J. & Savage, B. D. 1995, ApJS, 97, 1 10.1086/192133

[21]

Lodders, K. 2003, ApJ, 591, 1220 10.1086/375492

[22]

Mathis, J. S. 2000, ApJ, 544, 347 10.1086/317210

[23]

Morton, D. C. 2003, ApJS, 149, 205 10.1086/377639

[24]

Nicastro, F., et al. 2002, ApJ, 573, 157 10.1086/340489

[25]

Proffitt, C., et al. 2002, STIS Instrument Handbook, Ver. 6.0 (Baltimore: STScI)

[26]

Ransom, S. M., Cordes, J. M. & Eikenberry, S. S. 2003, ApJ, 589, 911 10.1086/374806

[27]

Ransom, S. M., Eikenberry, S. S. & Middleditch, J. 2002, AJ, 124, 1788 10.1086/342285

[28]

Ransom, S. M., Hessels, J., Stairs, I., Kaspi, V., Freire, P. & Backer, D. 2005, in ASP Conf. Ser. 328, Binary Radio Pulsars, ed. F. Rasio & I. Stairs (San Francisco: ASP), 199 10.1086/381730

[29]

Rasmussen, A., Kahn, S. M. & Paerels, F. 2003, in The IGM/Galaxy Connection: The Distribution of Baryons at \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $z=0$ \end{document} , ed. J. L. Rosenberg & M. E. Putman (Dordrecht: Kluwer), 109

[30]

Reynolds, R. J. 1989, ApJ, 345, 811 10.1086/167952

[31]

------. 1993, in AIP Conf. Proc. 278, Back to the Galaxy, ed. S. Holt & F. Verter (New York: AIP), 156

[32]

Reynolds, R. J., Hausen, N. R., Tufte, S. L. & Haffner, L. M. 1998, ApJ, 494, L99 10.1086/311154

[33]

Reynolds, R. J. & Tufte, S. L. 1995, ApJ, 439, L17 10.1086/187734

[34]

Savage, B. D., Drake, J. F., Budich, W. & Bohlin, R. C. 1977, ApJ, 216, 291 10.1086/155471

[35]

Savage, B. D. & Sembach, K. R. 1991, ApJ, 379, 245 10.1086/170498

[36]

INTERSTELLAR ABUNDANCES FROM ABSORPTION-LINE OBSERVATIONS WITH THE HUBBLE SPACE TELESCOPE

Blair D. Savage, Kenneth R. Sembach

Annual Review of Astronomy and Astrophysics 10.1146/annurev.astro.34.1.279

[37]

Savage, B. D., et al. 2000, ApJS, 129, 563 10.1086/313420

[38]

------. 2003, ApJS, 146, 125 10.1086/346229

[39]

Sembach, K. R., Howk, J. C., Ryans, R. S. I. & Keenan, F. P. 2000, ApJ, 528, 310 10.1086/308173

[40]

Sembach, K. R. & Savage, B. D. 1992, ApJS, 83, 147 10.1086/191734

[41]

------. 1996, ApJ, 457, 211 10.1086/176723

[42]

Sembach, K. R., et al. 2003, ApJS, 146, 165 10.1086/346231

[43]

Shull, J. M., et al. 2000, ApJ, 538, L73 10.1086/312782

[44]

Slavin, J. D., McKee, C. F. & Hollenbach, D. J. 2000, ApJ, 541, 218 10.1086/309409

[45]

Sonneborn, G., et al. 2002, ApJS, 140, 51 10.1086/339134

[46]

Spitzer, L. & Fitzpatrick, E. L. 1993, ApJ, 409, 299 10.1086/172664

[47]

Sutherland, R. S. & Dopita, M. A. 1993, ApJS, 88, 253 10.1086/191823

[48]

Wakker, B. P., et al. 2003, ApJS, 146, 1 10.1086/346230

[49]

Yao, Y. & Wang, Q. D. 2005, ApJ, 624, 751 10.1086/429537

Cited By

54

Sulphur chemistry in the L1544 pre-stellar core

Charlotte Vastel, D Quénard · 2018

Monthly Notices of the Royal Astron...

Metrics

54

Citations

49

References

Details

Published: Jan 20, 2006
Vol/Issue: 637(1)
Pages: 333-341

Authors

Center for Space Research, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139

B

Blair D. Savage

Department of Astronomy, University of Wisconsin, Madison, Wisconsin 53706

Cite This Article

J. Christopher Howk, Kenneth R. Sembach, Blair D. Savage (2006). A Method for Deriving Accurate Gas‐Phase Abundances for the Multiphase Interstellar Galactic Halo. The Astrophysical Journal, 637(1), 333-341. https://doi.org/10.1086/497352

A Method for Deriving Accurate Gas‐Phase Abundances for the Multiphase Interstellar Galactic Halo

You May Also Like