CI emission in Ultra Luminous Infrared Galaxies as a molecular gas mass tracer

Preprint English OPEN
Papadopoulos, Padeli P.; Greve, Thomas R.;
(2004)
  • Related identifiers: doi: 10.1086/426059
  • Subject: Astrophysics
    arxiv: Astrophysics::Galaxy Astrophysics | Astrophysics::Cosmology and Extragalactic Astrophysics

We present new sensitive wide-band measurements of the fine structure line 3^P_1 -> 3^P_0 (J=1-0, 492GHz) of neutral atomic carbon (CI) in the two typical Ultra Luminous Infrared Galaxies NGC6240 and Arp220. We then use them along with several other CI measurements in s... View more
  • References (11)
    11 references, page 1 of 2

    Aalto S., Booth R. S., Black J. M., & Johansson L. E. B. 1995 A&A, 300, 369 Bryant P. M., & Scoville N. Z. 1999, AJ, 117, 2632 Downes, D., Solomon, P. M. 1998, ApJ, 507, 615 Gao Y., & Solomon P. M. 2004, ApJS, 152, 63 Genzel R., Lutz D., Sturm E., Egami E., Kunze D., Moorrwood A. F. M., Rigopoulou D., Spoon H. W. W., Sternberg A., Tacconi-Garman L. E., Tacconi L., & Thatte N. 1998, ApJ, 498, 579

    Gerin M., & Phillips T. G. 1998, ApJ, 509, L17 Gerin M., & Phillips T. G. 2000, ApJ, 537, 644 Glenn J, & Hunter T. R. 2001, ApJS, 135, 177 Hughes D. H., et al. 1998, Nature, 394, 241 Ikeda M., Oka T., Tatematsu K., Sekimoto Y., Yamamoto S. 2002, ApJS, 139, 467 Keene J., Blake G. A., Phillips T. G., Huggins P. J., & Beichman C. A. 1985, ApJ, 299, 967 Keene J., Lis D. C., Phillips T. G., & Schilke P. 1997, in Molecules in astrophysics: probes & processes IAU Symposium No 178, ed. Ewine van Dishoeck (Cambridge: Cambridge Univ. Press) 129

    Lihong Yao, Seaquist E. R., Kuno N., & Dunne L. 2003, ApJ, 588, 771 Ojha R., Stark A. A., Hsieh H. H., Lane A. P., Chamberlin R. A., Bania T. M., Bolatto A. D., Jackson J. M., & Wright G. A. 2001, ApJ, 548, 253

    Papadopoulos P. P., Thi W.-F., & Viti S. 2004, MNRAS, 351, 147 Phillips T. G., & Huggins P. J. 1981, ApJ, 251, 533 Radford S. J. E, & Nyman L.-A. 2001, in ALMA Project Book, Chapter 14, (http://www.tuc.nrao.edu/mma/sites/)

    Sanders D. B., Soifer B. T., Elias J. H., Madore B. F., Matthews K., Neugebauer G., & Scoville N. Z. 1988, ApJ, 325, 74

    Schilke P., Carlstrom J. E., Keene J., & Phillips T. G. 1993, ApJ, 417, L67 Solomon P. M., Downes D., Radford S. J. E., & Barett J. W. 1997, ApJ, 478, 144 Smail I., Ivison R. J. I., & Blain A. W. 1997, ApJ, 490, L5 Tacconi L. J., Genzel R., Tecza M., Galimore J. F., Downes D., & Scoville N. Z. 1999, ApJ, 524, 732

    Tacconi L. J., Genzel R., Lutz D., Rigopoulou D., Baker A. J., Iserlohe C., & Tecza M. 2002, ApJ, 580, 73

    Tielens A. G. G. M., & Hollenbach D. 1985a, ApJ, 291, 722 Tielens A. G. G. M., & Hollenbach D. 1985b, ApJ, 291, 747 Weiss A., Henkel C., Downes D., & Walter F. 2003, A&A, 409, L41 White G. J., Ellison B., Claude S., Dent W. R. F., & Matheson D. N. 1994, A&A, 284, L23 Zhu M., Seaquist E. R., Davoust E., Frayer D. T., Bushouse H. A. 1999, AJ, 118, 145 NGC 6240d 0.024 600±180 (59, 103) 0.52 (6 ± 2) 4 Arp 220 0.018 1160±350 (64, 103-104) 0.47 (7 ± 2) 5 Mrk 231 0.042 200±55a (74, 3.5×103) 0.45 (7 ± 2) 4 NGC 6090e 0.029 270±55a (40, 103-104) 0.48 (4 ± 1) 6 10565+2448 0.043 500±150a (60, 1.2×103) 0.51 (16 ± 5) 4 a from Gerin & Phillips 2000

    b Solomon et al. 1997; Downes & Solomon 1998 (except NGC 6240, NGC 6090) c Downes & Solomon 1998 (except NGC 6240, NGC 6090)

    d MCO(H2) from Tacconi et al. 1999; (Tk, n) from Large Velocity Gradient modeling of the line ratios reported by Tacconi et al. and references therein.

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