The high-density ionized gas in the central parsec of the galaxy

Jun Hui Zhao, Ray Blundell, James M. Moran, Dennis Downes, Karl F. Schuster, Daniel P Marrone

Research output: Contribution to journalArticle

38 Citations (Scopus)

Abstract

We report a study of the H30α line emission at 1.3 mm from the region around Sgr A* made with the Submillimeter Array at a resolution of 2″ over a field of 60″ (2 pc) and a velocity range of -360 to +345 km s-1. This field encompasses most of the Galactic center's "minispiral." With an isothermal homogeneous H II model, we determined the physical conditions of the ionized gas at specific locations in the Northern and Eastern Arms from the H30α line data along with Very Large Array data from the H92α line at 3.6 cm and from the radio continuum emission at 1.3 cm. The typical electron density and kinetic temperature in the minispiral arms are 3-21 × 104 cm-3 and 5000-13,000 K, respectively. The H30α and H92α line profiles are broadened due to the large velocity shear within and along the beam produced by dynamical motions in the strong gravitational field near Sgr A*. We constructed a threedimensional model of the minispiral using the orbital parameters derived under the assumptions that the gas flows are in Keplerian motion. The gas in the Eastern Arm appears to collide with the Northern Arm flow in the "Bar" region, which is located 0.1-0.2 pc south of and behind Sgr A*. Finally, a total Lyman continuum flux of 3 × 1050 photons s-1 is inferred from the assumption that the gas is photoionized and the ionizing photons for the high-density gas in the minispiral arms are from external sources, which is equivalent to ∼250 O9-type zero-age-main-sequence stars.

Original languageEnglish (US)
Pages (from-to)1097-1109
Number of pages13
JournalAstrophysical Journal
Volume723
Issue number2
DOIs
StatePublished - Nov 10 2010
Externally publishedYes

Fingerprint

ionized gases
galaxies
continuums
Very Large Array (VLA)
main sequence stars
photons
gas density
gases
gas
gravitational fields
gas flow
shear
orbitals
kinetics
profiles
electron density
radio
temperature

Keywords

  • Galaxy: center
  • H II regions
  • ISM: individual objects (Sgr A)
  • ISM: kinematics and dynamics
  • Radio lines: ISM

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Zhao, J. H., Blundell, R., Moran, J. M., Downes, D., Schuster, K. F., & Marrone, D. P. (2010). The high-density ionized gas in the central parsec of the galaxy. Astrophysical Journal, 723(2), 1097-1109. https://doi.org/10.1088/0004-637X/723/2/1097

The high-density ionized gas in the central parsec of the galaxy. / Zhao, Jun Hui; Blundell, Ray; Moran, James M.; Downes, Dennis; Schuster, Karl F.; Marrone, Daniel P.

In: Astrophysical Journal, Vol. 723, No. 2, 10.11.2010, p. 1097-1109.

Research output: Contribution to journalArticle

Zhao, JH, Blundell, R, Moran, JM, Downes, D, Schuster, KF & Marrone, DP 2010, 'The high-density ionized gas in the central parsec of the galaxy', Astrophysical Journal, vol. 723, no. 2, pp. 1097-1109. https://doi.org/10.1088/0004-637X/723/2/1097
Zhao, Jun Hui ; Blundell, Ray ; Moran, James M. ; Downes, Dennis ; Schuster, Karl F. ; Marrone, Daniel P. / The high-density ionized gas in the central parsec of the galaxy. In: Astrophysical Journal. 2010 ; Vol. 723, No. 2. pp. 1097-1109.
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