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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents

ID: 421662.0, MPI für Astronomie / Publikationen_mpia
Absorption line survey of H+3 toward the Galactic center sources. II. Eight infrared sources within 30 pc of the Galactic center
Authors:Goto, Miwa; Usuda, Tomonori; Nagata, Tetsuya; Geballe, T. R.; McCall, Benjamin J.; Indriolo, Nick; Suto, Hiroshi; Henning, Thomas; Morong, Christopher P.; Oka, Takeshi
Date of Publication (YYYY-MM-DD):2008
Title of Journal:The Astrophysical Journal
Start Page:306
End Page:319
Review Status:Peer-review
Audience:Experts Only
Abstract / Description:Infrared absorption lines of H+3, including the metastable R(3,3)l line, have been observed toward eight bright infrared sources associated with hot and massive stars located in and between the Galactic center cluster and the Quintuplet cluster 30 pc to the east. The absorption lines with high-velocity dispersion arise in the Galaxy's central molecular zone (CMZ) as well as in foreground spiral arms. The temperature and density of the gas in the CMZ, as determined from the relative strengths of the H+3 lines, are T=200-300 K and n<=50-200 cm-3. The detection of high column densities of H+3 toward all eight stars implies that this warm and diffuse gaseous environment is widespread in the CMZ. The products of the ionization rate and path length for these sight lines are 1000 and 10 times higher than in dense and diffuse clouds in the Galactic disk, respectively, indicating that the ionization rate, zeta, is not less than 10-15 s-1 and that L is at least on the order of 50 pc. The warm and diffuse gas is an important component of the CMZ, in addition to the three previously known gaseous environments: (1) cold molecular clouds observed by radio emission of CO and other molecules; (2) hot (T=104-106 K) and highly ionized diffuse gas (ne=10-100 cm-3) seen in radio recombination lines, far infrared atomic lines, and radio-wave scattering; and (3) ultrahot (T=107-108 K) X-ray emitting plasma. Its prevalence significantly changes the understanding of the environment of the CMZ. The sight line toward GC IRS 3 is unique in showing an additional H+3 absorption component, which is interpreted as being due to either a cloud associated with circumnuclear disk or the ``50 km s-1 cloud'' known from radio observations. An infrared pumping scheme is examined as a mechanism to populate the (3,3) metastable level in this cloud. Based on data collected at Subaru Telescope, operated by the National Astronomical Observatory of Japan.
Free Keywords:Galaxy: Center; ISM: Clouds; ISM: Lines and Bands; ISM: Molecules; stars: individual (GC IRS 1W); stars: individual (GC IRS 21); stars: individual (GC IRS 3); stars: individual (GCS 3-2); stars: individual (NHS 21); stars: individual (NHS 22); stars: individual (NHS 25); stars: individual (NHS 42)
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL: [ID No:1]
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