Near-infrared integral field spectroscopy of Markarian 231

被引:25
|
作者
Krabbe, A
Colina, L
Thatte, N
Kroker, H
机构
[1] SPACE TELESCOPE SCI INST,BALTIMORE,MD 21218
[2] ESA,DEPT SPACE SCI,DIV ASTROPHYS,F-75738 PARIS 15,FRANCE
来源
ASTROPHYSICAL JOURNAL | 1997年 / 476卷 / 01期
关键词
galaxies; individual; (Markarian; 231); ISM; Seyfert; structure; infrared;
D O I
10.1086/303619
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The ultraluminous infrared Seyfert 1 galaxy Mrk 231 has been spectrally imaged in the K band with the new three-dimensional MPE integral held spectrometer. The combined images of the H-2 emission lines show, for the first time in an ultraluminous infrared galaxy, the presence of an extended circumnuclear structure of hot molecular gas. The H-2 emitting region has a size of similar to 2.4 kpc and a hot molecular gas mass M(H2)(hot) similar to 2 x 10(4) M circle dot. The H-2 emission-line ratios indicate that the gas is most likely thermally excited. If as in NGC 7469 star formation is associated with the H-2 emission, the starburst would have a far-IR luminosity L(FIR) similar to 1 x 10(12) L circle dot. This value represents an upper limit, since a fraction of the hot molecular gas may be excited by the radiation field emerging from the nucleus. The K-band three-dimensional data cube also shows for the first time the presence of extended narrow Pa alpha emission blueshifted by similar to 1400 km s(-1) with respect to the systemic velocity, and located similar to 0.6 kpc northwest of the nucleus. The detection of CO absorption bands with a spatial distribution peaking on the K-band continuum provides evidence for a central stellar concentration. The low CO spectroscopic index indicates, however, dilution by hot dust emission or by a nonthermal active galactic nucleus. The Pa alpha/H alpha ratio confirms previous extinction measurements based on Balmer line ratios, i.e., visual extinction of A(V) similar to 2.0-6.6 mag. The quasar-type nucleus of Mrk 231 should then be transparent at 2 mu m and also in hard X-rays. A weak nuclear He I lambda 2.058 mu m (He I/Pa alpha = 0.032) is detected, and no detection of [Si VI] lambda 1.962 mu m is made, placing an upper limit of 4 x 10(-18) Wm(-2) for the coronal gas emission. The ionizing source could either be a far-UV and X-ray quiet quasar or else a nuclear starburst with an upper mass limit greater than or equal to 60 M circle dot.
引用
收藏
页码:98 / 104
页数:7
相关论文
共 50 条
  • [1] NEAR-INFRARED IMAGING OF MARKARIAN-231
    KODAIRA, K
    OHTA, K
    UENO, M
    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 1992, 44 (06) : L247 - L251
  • [2] Integral field spectroscopy with the Gemini near-infrared spectrograph
    Allington-Smith, J
    Dubbeldam, CM
    Content, R
    Dunlop, CJ
    Robertson, DJ
    Elias, J
    Rodgers, B
    Turner, J
    GROUND-BASED INSTRUMENTATION FOR ASTRONOMY, PTS 1-3, 2004, 5492 : 701 - 710
  • [3] NEAR-INFRARED IMAGING OF MARKARIAN-231 - EVIDENCE FOR A DOUBLE NUCLEUS
    ARMUS, L
    SURACE, JA
    SOIFER, BT
    MATTHEWS, K
    GRAHAM, JR
    LARKIN, JE
    ASTRONOMICAL JOURNAL, 1994, 108 (01): : 76 - 83
  • [4] Integral field near-infrared spectroscopy of II Zw 40
    Vanzi, L.
    Cresci, G.
    Telles, E.
    Melnick, J.
    ASTRONOMY & ASTROPHYSICS, 2008, 486 (02) : 393 - 403
  • [5] Near-infrared integral field spectroscopy of massive young stellar objects
    Murakawa, K.
    Lumsden, S. L.
    Oudmaijer, R. D.
    Davies, B.
    Wheelwright, H. E.
    Hoare, M. G.
    Ilee, J. D.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2013, 436 (01) : 511 - 525
  • [6] Near-infrared integral field spectroscopy of star-forming galaxies
    Dale, DA
    Roussel, H
    Contursi, A
    Helou, G
    Dinerstein, HL
    Hunter, DA
    Hollenbach, DJ
    Egami, E
    Matthews, K
    Murphy, TW
    Lafon, CE
    Rubin, RH
    ASTROPHYSICAL JOURNAL, 2004, 601 (02): : 813 - 830
  • [7] Near-infrared integral-field spectroscopy of violent starburst environments
    de Grijs, R
    NEW ASTRONOMY REVIEWS, 2006, 49 (10-12) : 495 - 500
  • [8] Near-infrared integral field spectroscopy of damped Lyman-α systems
    Bunker, A
    Ferguson, A
    Johnson, R
    McMahon, R
    Parry, I
    Pettini, M
    Aragón-Salamanca, A
    Somerville, R
    DEEP FIELDS, 2001, : 330 - 333
  • [9] Near-infrared integral field spectroscopy of damped Lyman-α systems
    Bunker, A
    Ferguson, A
    Johnson, R
    McMahon, R
    Parry, I
    Pettini, M
    Aragón-Salamanca, A
    Somerville, R
    MINING THE SKY, 2001, : 214 - 217
  • [10] Near-infrared integral-field spectroscopy of the companion to GQ Lupi
    Seifahrt, A.
    Neuhaeuser, R.
    Hauschildt, P. H.
    ASTRONOMY & ASTROPHYSICS, 2007, 463 (01) : 309 - 313