Results 1 to 10 of about 9,232 (192)
Astrochemistry of sub-millimeter sources in Orion [PDF]
, 2003 Cornerstone molecules (CO, H_2CO, CH_3OH, HCN, HNC, CN, CS, SO) were observed
toward seven sub-millimeter bright sources in the Orion molecular cloud in
order to quantify the range of conditions for which individual molecular line
tracers provide ...Doug Johnstone, A. M. S. Boonman, E. F. van Dishoeck +2 moreopenalex +5 more sourcesAstrochemistry: overview and challenges [PDF]
, 2017 This paper provides a brief overview of the journey of molecules through the
Cosmos, from local diffuse interstellar clouds and PDRs to distant galaxies,
and from cold dark clouds to hot star-forming cores, protoplanetary disks,
planetesimals and ...van Dishoeck, Ewine F.core +3 more sourcesRecommended Thermal Rate Coefficients for the C + H$_3^+$ Reaction and
Some Astrochemical Implications [PDF]
, 2016 We have incorporated our experimentally derived thermal rate coefficients for
C + H$_3^+$ forming CH$^+$ and CH$_2^+$ into a commonly used astrochemical
model.Buzard, C. F., de Ruette, N., Miller, K. A., O'Connor, A. P., Savin, D. W., Urbain, X., Vissapragada, S. +6 morecore +3 more sourcesGrain Surface Models and Data for Astrochemistry [PDF]
, 2017 The cross-disciplinary field of astrochemistry exists to understand the formation, destruction, and survival of molecules in astrophysical environments. Molecules in space are synthesized via a large variety of gas-phase reactions, and reactions on dust ...A. Al-Halabi, A. Al-Halabi, A. Al-Halabi, A. Bacmann, A. Belloche, A. Belloche, A. Dalgarno, A. Dutrey, A. Leger, A. Lipshtat, A. McKellar, A. Nagaoka, A. Nagaoka, A. Pedersen, A. Rimola, A. Stutz, A. Tielens, A. Wolff, A.A. Boogert, A.E. Douglas, A.G.G.M. Tielens, A.G.G.M. Tielens, A.G.G.M. Tielens, A.I. Vasyunin, A.I. Vasyunin, A.S. Bolina, A.S. Bolina, A.S. Bolina, A.S. Eddington, A.V. Ivlev, B. Lepetit, B.T. Draine, B.T. Draine, C. Arasa, C. Arasa, C. Arasa, C. Chyba, C. Eckart, C. Vastel, C. Walsh, C. Walsh, C.M. Leung, D. Field, D. Hollenbach, D. McElroy, D. Semenov, D. Semenov, D.A. Adriaens, D.E. Woon, D.H. Parker, D.J. Hollenbach, D.P. Ruffle, D.P. Ruffle, D.R. Bates, D.T. Gillespie, E. Anders, E. Congiu, E. Gonzalez-Lavado, E. Herbst, E. Herbst, E. Herbst, E. Herbst, E. Herbst, E. M. Penteado, E. Wigner, E.A. Bergin, E.C. Fayolle, E.C. Fayolle, E.C. Fayolle, E.F. Dishoeck van, E.F. Dishoeck van, E.K. Campbell, E.M. Penteado, E.R. Batista, F. Dulieu, F. Mispelaer, F.L. Schöier, G. Cooper, G. Fedoseev, G. Nyman, G.A. Cruz-Diaz, G.A. Cruz-Diaz, G.A. Cruz-Diaz, G.M. Muñoz Caro, G.W. Fuchs, G.W. Fuchs, H. Chaabouni, H. Hidaka, H. Hidaka, H. Hidaka, H. Linnartz, H. M. Cuppen, H.J. Fraser, H.J. Fraser, H.M. Cuppen, H.M. Cuppen, H.M. Cuppen, J. Bossa, J. Cami, J. Cernicharo, J. Fillion, J. Gonzalez, J. He, J. He, J. Kalvāns, J. Koning, J. Kästner, J. Zhen, J.A. Noble, J.A. Noble, J.A. Noble, J.B. Bergner, J.B. Bossa, J.E. Elsila, J.K. Jørgensen, J.M.C. Rawlings, J.R. Burke, K. Acharyya, K. Acharyya, K. Furuya, K. Furuya, K. Hiraoka, K. Hiraoka, K. Hiraoka, K. Hiraoka, K. Isokoski, K. Kuwahata, K. Kvenvolden, K. Willacy, K. Willacy, K.I. Öberg, K.I. Öberg, K.I. Öberg, K.I. Öberg, K.I. Öberg, K.I. Öberg, K.I. Öberg, K.I. Öberg, K.J. Chuang, K.M. Pontoppidan, K.M. Pontoppidan, L. Allamandola, L. Amiaud, L.B. D’Hendecourt, L.B. D’Hendecourt, L.B. D’Hendecourt, L.E. Snyder, L.J. Karssemeijer, L.J. Karssemeijer, L.J. Karssemeijer, L.J. Karssemeijer, L.T. Greenberg, M. Accolla, M. Agúndez, M. Allen, M. Bertin, M. Bertin, M. Bertin, M. Minissale, M. Minissale, M. Monge-Palacios, M. Monge-Palacios, M.B. Bell, M.C. Hemert van, M.P. Collings, M.P. Collings, M.P. Collings, M.S. Westley, M.S. Westley, N. Balucani, N. Katz, N. Lippok, N. Miyauchi, N. Nishi, N. Watanabe, N. Watanabe, N. Watanabe, N. Watanabe, N.F.W. Ligterink, N.G. Adams, N.J. Mason, N.J.B. Green, O. Berné, O. Biham, P. Caselli, P. Ehrenfreund, P. Swings, P. Theule, P.A. Gerakines, P.D. Brown, P.M. Woods, Q. Chang, Q. Chang, Q. Chang, Q. Chang, R. Garrod, R. Launhardt, R. T. Garrod, R.E. Weston, R.J. Gould, R.J.A. Grim, R.M. Logan, R.P. Bell, R.T. Garrod, R.T. Garrod, R.T. Garrod, R.T. Garrod, R.T. Garrod, R.T. Garrod, R.T. Garrod, S. Andersson, S. Andersson, S. Andersson, S. Andersson, S. Cazaux, S. Ioppolo, S. Ioppolo, S. Viti, S.A. Sandford, S.A. Sandford, S.A. Sandford, S.A. Sandford, S.B. Charnley, S.B. Charnley, S.D. Green, S.E. Bisschop, S.E. Bisschop, S.S. Prasad, T. Albertsson, T. Butscher, T. Grassi, T. Hama, T. Hama, T. Hama, T. Henning, T. Lamberts, T. Lamberts, T. Lamberts, T. Lamberts, T. Lamberts, T. Lamberts, T. Lauck, T. Stantcheva, T. Stantcheva, T.I. Hasegawa, T.I. Hasegawa, T.I. Hasegawa, T.J. Millar, T.J.H. Hele, T.L. Nguyen, T.L. Nguyen, T.L. Nguyen, T.L. Nguyen, T.P.M. Goumans, T.P.M. Goumans, T.P.M. Goumans, T.P.M. Goumans, T.W. Hartquist, V. Barone, V. Buch, V. Pirronello, V. Pirronello, V. Pirronello, V. Taquet, V. Taquet, V. Wakelam, V. Wakelam, V.K. Veeraghattam, W. Hagen, W.A. Brown, W.D. Geppert, W.D. Watson, W.D. Watson, W.D. Watson, Y. Aikawa, Y. Chen, Y. Li, Y. Oba, Y. Oba, Y. Oba, Y. Oba, Y. Oba, Y. Zhang, Y.V. Suleimanov, Z. Awad +284 morecore +6 more sourcesOn the Energetics of the HCO$^+$ + C $\to$ CH$^+$ + CO Reaction and Some
Astrochemical Implications [PDF]
, 2017 We explore the energetics of the titular reaction, which current
astrochemical databases consider open at typical dense molecular (i.e., dark)
cloud conditions.Bhaskar, Roshan G., Savin, Daniel W., Urbain, Xavier, Vissapragada, Shreyas +3 morecore +3 more sourcesAstrochemistry and Astrophotonics for an Antarctic Observatory
, 2009 Due to its location and climate, Antarctica offers unique conditions for
long-period observations across a broad wavelength regime, where important
diagnostic lines for molecules and ions can be found, that are essential to
understand the chemical ...A. Kelz, Beitz, Bland-Hawthorn, Bland-Hawthorn, Bland-Hawthorn, Ehrenfreund, Fulara, H.-G. Löhmannsröben, Kelz, Lawrence, M. Kumke, M.M. Roth, Maier, Mandon, Murphy, Noordegraaf, Snow, Thomson +17 morecore +1 more sourceA hybrid moment equation approach to gas-grain chemical modeling [PDF]
, 2011 [Context] The stochasticity of grain chemistry requires special care in
modeling. Previously methods based on the modified rate equation, the master
equation, the moment equation, and Monte Carlo simulations have been used.
[Aims] We attempt to develop a Awad, B. Parise, Barzel, Barzel, Barzel, Biham, Biham, Caselli, Chang, Charnley, Charnley, Charnley, Charnley, Cuppen, F. Du, Garrod, Garrod, Garrod, Gillespie, Gillespie, Gillespie, Gillespie, Green, Hasegawa, Hasegawa, Lipshtat, Mattis, McQuarrie, Menten, Ohkubo, Rae, Stantcheva, Stantcheva, Stantcheva, Tielens, Tielens, Vasyunin, Vasyunin, Woodall +38 morecore +2 more sources