Abstract
Observations of the molecular cloud G1.6-0.025 in the 2K-1K and J 0-J −1 E series and 5−1-40 E line of CH3OH, the (2-1) and (3-2) lines of SiO, and the 7−7-6−6 line of HNCO are described. Maps of the previously observed extended cloud with V lsr∼50 km/s and high-velocity clump with V lsr∼160 km/s, as well as a newly detected clump with V lsr∼0 km/s, have been obtained. The extended cloud and high-velocity clump have a nonuniform structure. The linewidths associated with all the objects are between 20 and 35 km/s, as is typical of clouds of the Galactic center. In some directions, emission at velocities from 40 to 160 km/s and from −10 to +75 km/s is observed at the clump boundaries, testifying to a connection between the extended cloud and the high-velocity clump and clump at V lsr∼0 km/s. Compact maser sources are probaby contributing appreciably to the emission of the extended cloud in the 5−1-40 E CH3OH line. Non-LTE modeling of the methanol emission shows that the extended cloud and high-velocity clump have a relatively low hydrogen density (<104 cm−3). The specific column density of methanol in the extended cloud exceeds 6×108 cm−3s, and is 4×108−6×109 cm−3s in the high-velocity clump. The kinetic temperatures of the extended cloud and high-velocity clump are estimated to be <80 K and 150–200 K, respectively. Possible mechanisms that can explain the link between the extended cloud with V lsr∼50 km/s and the clumps with V lsr∼0 km/s and ∼160 km/s are briefly discussed.
Similar content being viewed by others
References
J. B. Whiteoak and F. F. Gardner, Mon. Not. R. Astron. Soc. 188, 445 (1979).
F. F. Gardner, J. B. Whiteoak, J. R. Forster, et al., Proc. Astron. Soc. Aust. 6, 176 (1985).
F. F. Gardner and F. Boes, Proc. Astron. Soc. Aust. 7, 185 (1987).
J. Bally, A. A. Stark, R. W. Wilson, and C. Hencel, Astrophys. J., Suppl. Ser. 65, 13 (1987).
M. Tsuboi, T. Handa, and N. Ukita, Astrophys. J., Suppl. Ser. 120(1), 1 (1999).
C. W. Lee, Astrophys. J., Suppl. Ser. 105, 129 (1996).
J. B. Whiteoak and R.-S. Peng, Mon. Not. R. Astron. Soc. 239, 677 (1989).
A. D. Haschick and W. A. Baan, Astrophys. J. 410, 663 (1993).
G. Dahmen, S. Huttemeister, and W. L. Duschl, The Central Regions of the Galaxies (IAU Symp. 184), p. 95.
S. Pak, D. T. Jaffe, and L. D. Keller, Astrophys. J. Lett. 457, L43 (1996).
S. Pak, private communication.
I. I. Berulis, S. V. Kalenski, A. M. Sobolev, and V. S. Strelnitski, Astron. Astrophys. Trans. 1, 231 (1992).
A. M. Sobolev, Astron. Zh. 69(6), 1148 (1992) [Sov. Astron. 36, 590 (1992)].
S. Saito, H. Mikami, S. Yamamoto, et al., Astron. Soc. Pac. Conf. Ser. 59, 241 (1994).
T. W. Hartquist, K. M. Menten, S. Lepp, and A. Dalgarno, Mon. Not. R. Astron. Soc. 272(1), 184 (1995).
Y-J. Kuan and L. E. Snyder, Astrophys. J. 470, 981 (1996).
P. Schilke, C. M. Walmsley, G. Pineau des Forêts, and D. R. Flower, Astron. Astrophys. 321, 293 (1997).
P. Caselli, T. W. Hartquist, and O. Havnes, Astron. Astrophys. 322, 296 (1997).
V. I. Slysh, S. V. Kalenski, and I. E. Val’tts, Astrophys. J. 442(2), 668 (1995).
J. L. Caswell, Yi. Jiyune, R. S. Booth, and D. M. Cragg, Mon. Not. R. Astron. Soc. 313(3), 599 (2000).
W. Batrla and K. M. Menten, Astrophys. J. Lett. 329(1), L117 (1988).
A. M. Sobolev, Astron. Tsirk., No. 1543, 7 (1990).
S. V. Kalenskii, V. I. Slysh, I. E. Val’tts, et al., Astron. Zh. 78, 31 (2001) [Astron. Rep. 45, 26 (2001)].
R. Mauersberger, C. Henkel, T. L. Wilson, and C. M. Walmsley, Astron. Astrophys. 162, 199 (1986).
Y. Cao, S. Therebey, T. A. Prince, and C. A. Beichman, http://irsa.ipac.caltech.edu/applications/IGA/ (1997).
R. Cesaroni and C. M. Walmsley, Astron. Astrophys. 241(2), 537 (1991).
P. A. Voinovich and A. D. Chernin, Pis’ma Astron. Zh. 21(6), 926 (1995) [Astron. Lett. 21, 835 (1995)].
A. D. Chernin, New Astron. 5(6), 327 (2000).
C. M. Durtra and E. Bica, Astron. Astrophys. 359, L9 (2000).
Author information
Authors and Affiliations
Additional information
__________
Translated from Astronomicheski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l}\) Zhurnal, Vol. 79, No. 12, 2002, pp. 1059–1073.
Original Russian Text Copyright © 2002 by Sali\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l}\), Sobolev, Kalinina.
Rights and permissions
About this article
Cite this article
Salii, S.V., Sobolev, A.M. & Kalinina, N.D. Shock tracers in the molecular cloud G1.6-0.025. Astron. Rep. 46, 955–968 (2002). https://doi.org/10.1134/1.1529254
Received:
Accepted:
Issue Date:
DOI: https://doi.org/10.1134/1.1529254