Universität zu Köln

Armijos-Abendano, J., Martin-Pintado, J., Requena-Torres, M. A., Gonzalez-Alfonso, E., Guesten, R., Weiss, A., Harris, A., I, Israel, F. P., Kramer, C., Stutzki, J. and van der Werf, P. (2019). Herschel water maps towards the vicinity of the black hole Sgr A. Astron. Astrophys., 624. LES ULIS CEDEX A: EDP SCIENCES S A. ISSN 1432-0746

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Abstract

Aims. We study the spatial distribution and kinematics of water emission in a similar to 8 x 8 pc(2) region of the Galactic center (GC) that covers the main molecular features around the supermassive black hole Sagittarius A* (Sgr A*). We also analyze the water excitation to derive the physical conditions and water abundances in the circumnuclear disk (CND) and the quiescent clouds. Methods. We presented the integrated line intensity maps of the ortho 1(10) - 1(01), and para 2(02) - 1(11) and 1(11) - 0(00) water transitions observed using the On the Fly mapping mode with the Heterodyne Instrument for the Far Infrared (HIFI) on board Herschel. To study the water excitation, we used HIFI observations of the ground state ortho and para (H2O)-O-18 transitions toward three selected positions in the vicinity of Sgr A*. In our study, we also used dust continuum measurements of the CND, obtained with the Spectral and Photometric Imaging REceiver (SPIRE) instrument. Using a non-local thermodynamical equilibrium (LTE) radiative transfer code, the water line profiles and dust continuum were modeled, deriving H2O abundances (XH2O), turbulent velocities (V-t), and dust temperatures (T-d). We also used a rotating ring model to reproduce the CND kinematics represented by the position velocity (PV) diagram derived from para 2(02) - 1(11) H2O lines. Results. In our H2O maps we identify the emission associated with known features around Sgr A*: CND, the Western Streamer, and the 20 and 50 km s(-1) clouds. The ground-state ortho water maps show absorption structures in the velocity range of [-220,10] km s 1 associated with foreground sources. The PV diagram reveals that the 2(02) - 1(11) H2O emission traces the CND also observed in other high-dipole molecules such as SiO, HCN, and CN. Using the non-LTE code, we derive high XH2O of similar to (0.1-1.3) x 10(-5), V-t of 14-23 km s(-1), and T-d of 15-45 K for the CND, and the lower XH2O of 4 x 10(-8) and V-t of 9 km s(-1) for the 20 km s(-1) cloud. Collisional excitation and dust effects are responsible for the water excitation in the southwest lobe of the CND and the 20 km s(-1) cloud, whereas only collisions can account for the water excitation in the northeast lobe of the CND. We propose that the water vapor in the CND is produced by grain sputtering by shocks of 10-20 km s(-1), with some contribution of high temperature and cosmic-ray chemistries plus a photon-dominated region chemistry, whereas the low XH2O derived for the 20 km s(-1) cloud could be partially a consequence of the water freeze-out on grains.

Item Type:	Journal Article
Creators:	Creators Email ORCID ORCID Put Code Armijos-Abendano, J. UNSPECIFIED UNSPECIFIED UNSPECIFIED Martin-Pintado, J. UNSPECIFIED UNSPECIFIED UNSPECIFIED Requena-Torres, M. A. UNSPECIFIED UNSPECIFIED UNSPECIFIED Gonzalez-Alfonso, E. UNSPECIFIED UNSPECIFIED UNSPECIFIED Guesten, R. UNSPECIFIED UNSPECIFIED UNSPECIFIED Weiss, A. UNSPECIFIED UNSPECIFIED UNSPECIFIED Harris, A., I UNSPECIFIED UNSPECIFIED UNSPECIFIED Israel, F. P. UNSPECIFIED UNSPECIFIED UNSPECIFIED Kramer, C. UNSPECIFIED UNSPECIFIED UNSPECIFIED Stutzki, J. UNSPECIFIED UNSPECIFIED UNSPECIFIED van der Werf, P. UNSPECIFIED UNSPECIFIED UNSPECIFIED
URN:	urn:nbn:de:hbz:38-150466
DOI:	10.1051/0004-6361/201833897
Journal or Publication Title:	Astron. Astrophys.
Volume:	624
Date:	2019
Publisher:	EDP SCIENCES S A
Place of Publication:	LES ULIS CEDEX A
ISSN:	1432-0746
Language:	English
Faculty:	Unspecified
Divisions:	Unspecified
Subjects:	no entry
Uncontrolled Keywords:	Keywords Language MASSIVE STAR-FORMATION; SAGITTARIUS-A-EAST; WARM MOLECULAR GAS; CENTRAL 2 PARSECS; GALACTIC-CENTER; LINE EMISSION; SIO EMISSION; IONIZED-GAS; DYNAMICS; CO Multiple languages Astronomy & Astrophysics Multiple languages
Refereed:	Yes
URI:	http://kups.ub.uni-koeln.de/id/eprint/15046