Abstract
The collisional pumping of H\({}_{2}\)O and СH\({}_{3}\)OH masers in magnetohydrodynamic nondissociative C-type shocks is considered. A grid of C-type shock models with speeds in the range 5–70 km s\({}^{-1}\) and preshock gas densities \(n_{\textrm{H}_{2},0}=10^{4}\)–\(10^{7}\) cm\({}^{-3}\) is constructed. The large velocity gradient approximation is used to solve the radiative transfer equation in molecular lines. The para-H\({}_{2}\)O 183.3 GHz and ortho-H\({}_{2}\)O 380.1 and 448.0 GHz transitions are shown to be inverted and to have an optical depth along the shock velocity \(|\tau|\sim 1\) at relatively low gas densities in the maser zone, \(n_{\textrm{H}_{2}}\gtrsim 10^{5}\)–\(10^{6}\) cm\({}^{-3}\). Higher gas densities, \(n_{\textrm{H}_{2}}\gtrsim 10^{7}\) cm\({}^{-3}\), are needed for efficient pumping of the remaining H\({}_{2}\)O masers. Simultaneous generation of H\({}_{2}\)O and class I СH\({}_{3}\)OH maser emission in a shock is possible at preshock gas densities \(n_{\textrm{H}_{2},0}\approx 10^{5}\) cm\({}^{-3}\) and shock speeds in the range \(u_{\textrm{s}}\approx 17.5{-}22.5\) km s\({}^{-1}\). The possibility of detecting class I СH\({}_{3}\)OH and para-H\({}_{2}\)O 183.3 GHz masers in star-forming regions and near supernova remnants is investigated.
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REFERENCES
A. C. A. Boogert, P. A. Gerakines, and D. C. B. Whittet, Ann. Rev. Astron. Astrophys. 53, 541 (2015).
J. Cernicharo, C. Thum, H. Hein, D. John, P. Garcia, and F. Mattioco, Astron. Astrophys. 231, L15 (1990).
J. Cernicharo, E. González-Alfonso, J. Alcolea, R. Bachiller, and D. John, Astrophys. J. 432, L59 (1994).
J. Cernicharo, R. Bachiller, and E. González-Alfonso, Astron. Astrophys. 305, L5 (1996).
J. Cernicharo, J. R. Pardo, E. González-Alfonso, E. Serabyn, T. G. Phillips, D. J. Benford, and D. Mehringer, Astrophys. J. 520, L131 (1999).
M. J. Claussen, W. M. Goss, and D. A. Frail, Astron. J. 117, 1387 (1999).
R. M. Crutcher, B. Wandelt, C. Heiles, E. Falgarone, and T. H. Troland, Astrophys. J. 725, 466 (2010).
A. Dalgarno, Proc. Natl. Acad. Sci. U. S. A. 103, 12269 (2006).
F. Daniel and J. Cernicharo, Astron. Astrophys. 553, A70 (2013).
F. Daniel, A. Faure, P. J. Dagdigian, M.-L. Dubernet, F. Lique, and G. Pineau des Forêts, Mon. Not. R. Astron. Soc. 446, 2312 (2015).
E. F. van Dishoeck, E. Herbst, and D. A. Neufeld, Chem. Rev. 113, 9043 (2013).
S. D. Doty, Astrophys. J. 535, 907 (2000).
B. T. Draine and C. F. McKee, Ann. Rev. Astron. Astrophys. 31, 373 (1993).
A. E. Dudorov, Sov. Astron. 35, 342 (1991).
M. Elitzur, D. J. Hollenbach, and C. F. McKee, Astrophys. J. 346, 983 (1989).
M. Emprechtinger, D. C. Lis, R. Rolffs, P. Schilke, R. R. Monje, C. Comito, C. Ceccarelli, D. A. Neufeld, et al., Astrophys. J. 765, 61 (2013).
A. Faure and E. Josselin, Astron. Astrophys. 492, 257 (2008).
A. Faure, N. Crimier, C. Ceccarelli, P. Valiron, L. Wiesenfeld, and M. L. Dubernet, Astron. Astrophys. 472, 1029 (2007).
D. R. Flower and G. Pineau des Forêts, Mon. Not. R. Astron. Soc. 406, 1745 (2010).
R. Genzel, M. J. Reid, J. M. Moran, and D. Downes, Astrophys. J. 244, 884 (1981).
I. E. Gordon, L. S. Rothman, R. J. Hargreaves, R. Hashemi, E. V. Karlovets, F. M. Skinner, E. K. Conway, C. Hill, et al., J. Quant. Spectrosc. Radiat. Transfer 277, 107949 (2022).
M. D. Gray, A. Baudry, A. M. S. Richards, E. M. L. Humphreys, A. M. Sobolev, and J. A. Yates, Mon. Not. R. Astron. Soc. 456, 374 (2016).
M. D. Gray, S. Etoka, A. M. S. Richards, and B. Pimpanuwat, Mon. Not. R. Astron. Soc. 513, 1354 (2022).
S. Green, S. Maluendes, and A. D. McLean, Astrophys. J. Suppl. Ser. 85, 181 (1993).
T. W. Hartquist, K. M. Menten, S. Lepp, and A. Dalgarno, Mon. Not. R. Astron. Soc. 272, 184 (1995).
I. M. Hoffman, W. M. Goss, C. L. Brogan, and M. J. Claussen, Astrophys. J. 627, 803 (2005).
D. Hollenbach, M. Elitzur, and C. F. McKee, Astrophys. J. 773, 70 (2013).
D. G. Hummer and G. B. Rybicki, Astrophys. J. 293, 258 (1985).
M. J. Kaufman and D. A. Neufeld, Astrophys. J. 456, 250 (1996a).
M. J. Kaufman and D. A. Neufeld, Astrophys. J. 456, 611 (1996b).
T. A. van Kempen, D. Wilner, and M. Gurwell, Astrophys. J. 706, L22 (2009).
S. König, S. Martín, S. Muller, J. Cernicharo, K. Sakamoto, L. K. Zschaechner, E. M. L. Humphreys, T. Mroczkowski, et al., Astron. Astrophys. 602, A42 (2017).
C.-Y. Kuo, S. H. Suyu, V. Impellizzeri, and J. A. Braatz, Publ. Astron. Soc. Jpn. 71, 57 (2019).
S. Leurini, K. M. Menten, and C. M. Walmsley, Astron. Astrophys. 592, A31 (2016).
B. C. McEwen, Y. M. Pihlström, and L. O. Sjouwerman, Astrophys. J. 793, 133 (2014).
B. C. McEwen, Y. M. Pihlström, and L. O. Sjouwerman, Astrophys. J. 826, 189 (2016).
L. Moscadelli, L. Testi, R. S. Furuya, C. Goddi, M. Claussen, Y. Kitamura, and A. Wootten, Astron. Astrophys. 446, 985 (2006).
A. V. Nesterenok, Astron. Lett. 39, 717 (2013).
A. V. Nesterenok, Mon. Not. R. Astron. Soc. 455, 3978 (2016).
A. V. Nesterenok, Astrophys. Space Sci. 363, 151 (2018).
A. V. Nesterenok, Astron. Lett. 46, 449 (2020).
A. V. Nesterenok, J. Phys.: Conf. Ser. 2103, 012012 (2021).
A. V. Nesterenok, Mon. Not. R. Astron. Soc. 509, 4555 (2022).
A. V. Nesterenok and D. A. Varshalovich, Astron. Lett. 37, 456 (2011).
A. V. Nesterenok, D. Bossion, Y. Scribano, and F. Lique, Mon. Not. R. Astron. Soc. 489, 4520 (2019).
D. A. Neufeld and G. J. Melnick, Astrophys. J. 368, 215 (1991).
D. A. Neufeld, G. J. Melnick, M. J. Kaufman, H. Wiesemeyer, R. Güsten, A. Kraus, K. M. Menten, O. Ricken, et al., Astrophys. J. 843, 94 (2017).
G. N. Ortiz-León, S. A. Dzib, M. A. Kounkel, L. Loinard, A. J. Mioduszewski, L. F. Rodríguez, R. M. Torres, G. Pech, et al., Astrophys. J. 834, 143 (2017).
M. Pereira-Santaella, E. González-Alfonso, A. Usero, S. García-Burillo, J. Martín-Pintado, L. Colina, A. Alonso-Herrero, S. Arribas, et al., Astron. Astrophys. 601, L3 (2017).
Y. M. Pihlström, L. O. Sjouwerman, D. A. Frail, M. J. Claussen, R. A. Mesler, and B. C. McEwen, Astron. J. 147, 73 (2014).
L. F. Rodríguez, G. Anglada, J. M. Torrelles, J. E. Mendoza-Torres, A. D. Haschick, and P. T. P. Ho, Astron. Astrophys. 389, 572 (2002).
S. V. Salii, A. M. Sobolev, and N. D. Kalinina, Astron. Rep. 46, 955 (2002).
C. N. Shingledecker, J. B. Bergner, R. Le Gal, K. I. Öberg, U. Hincelin, and E. Herbst, Astrophys. J. 830, 151 (2016).
V. S. Strelnitskii, Sov. Phys. Usp. 17, 507 (1975)].
D. A. Varshalovich, A. V. Ivanchik, and N. S. Babkovskaya, Astron. Lett. 32, 29 (2006).
M. A. Voronkov, J. L. Caswell, S. P. Ellingsen, J. A. Green, and S. L. Breen, Mon. Not. R. Astron. Soc. 439, 2584 (2014).
N. Watanabe and A. Kouchi, Astrophys. J. 571, L173 (2002).
J. M. Woodall and M. D. Gray, Mon. Not. R. Astron. Soc. 378, L20 (2007).
C. Yang, E. González-Alfonso, A. Omont, M. Pereira-Santaella, J. Fischer, A. Beelen, and R. Gavazzi, Astron. Astrophys. 634, L3 (2020).
J. A. Yates, D. Field, and M. D. Gray, Mon. Not. R. Astron. Soc. 285, 303 (1997).
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Nesterenok, A.V. Collisional Pumping of H\({}_{2}\)O and СH\({}_{3}\)OH Masers in C-Type Shock Waves. Astron. Lett. 48, 345–359 (2022). https://doi.org/10.1134/S1063773722060044
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DOI: https://doi.org/10.1134/S1063773722060044