au.\*:("HASEGAWA, T. I")
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Hydrostatic models of Bok globulesHASEGAWA, T. I.Publications of the Astronomical Society of Japan. 1988, Vol 40, Num 2, pp 219-247, issn 0004-6264Article
New gas-grain chemical models of quiescent dense interstellar clouds: the effects of H2 tunnelling reactions and cosmic ray induced desorptionHASEGAWA, T. I; HERBST, E.Monthly Notices of the Royal Astronomical Society. 1993, Vol 261, Num 1, pp 83-102, issn 0035-8711Article
Three-phase chemical models of dense interstellar clouds: gas, dust particle mantles and dust particle surfacesHASEGAWA, T. I; HERBST, E.Monthly Notices of the Royal Astronomical Society. 1993, Vol 263, Num 3, pp 589-606, issn 0035-8711Article
A spectral line survey of Orion KL in the bands 486-492 and 541-577 GHz with the Odin* satellite** II. Data analysisPERSSON, C. M; OLOFSSON, A. O. H; KWOK, S et al.Astronomy and astrophysics (Berlin. Print). 2007, Vol 476, Num 2, pp 807-828, issn 0004-6361, 22 p.Article
A spectral line survey of Orion KL in the bands 486-492 and 541-577 GHz with the Odin* satellite** I. The observational dataOLOFSSON, A. O. H; PERSSON, C. M; KWOK, S et al.Astronomy and astrophysics (Berlin. Print). 2007, Vol 476, Num 2, pp 791-806, issn 0004-6361, 16 p.Article
Models of gas-grain chemistry in dense interstellar clouds with complex organic moleculesHASEGAWA, T. I; HERBST, E; CHUN MING LEUNG et al.The Astrophysical journal. Supplement series. 1992, Vol 82, Num 1, pp 167-195, issn 0067-0049Article
Properties of the molecular cloud about S140 IRS 1 deduced from HCO+ J = 3→2 observationsHASEGAWA, T. I; MITCHELL, G. F; HENRIKSEN, R. N et al.The Astronomical journal (New York). 1991, Vol 102, Num 2, pp 666-675, issn 0004-6256, 10 p.Article
First detection of CO lines in a water fountain starHE, J. H; IMAI, H; HASEGAWA, T. I et al.Astronomy and astrophysics (Berlin. Print). 2008, Vol 488, Num 2, issn 0004-6361, L21-L24Article
Chemical differentiation between star-forming regions : the Orion Hot Core and Compact RidgeCASELLI, P; HASEGAWA, T. I; HERBST, E et al.The Astrophysical journal. 1993, Vol 408, Num 2, pp 548-558, issn 0004-637X, 1Article
A CO J = 2 → 1 study of the outflow sources GL 490, 2591, M8E-IR, and W3 IRS 5MITCHELL, G. F; HASEGAWA, T. I; SCHELLA, J et al.The Astrophysical journal. 1992, Vol 386, Num 2, pp 604-617, issn 0004-637X, p.1Article
Episodic outflows from high-mass protostarsMITCHELL, G. F; MAILLARD, J.-P; HASEGAWA, T. I et al.The Astrophysical journal. 1991, Vol 371, Num 1, pp 342-356, issn 0004-637X, 15 p., p.1Article
Observations of HCO+ in B335HASEGAWA, T. I; ROGERS, C; HAYASHI, S. S et al.The Astrophysical journal. 1991, Vol 374, Num 1, pp 177-185, issn 0004-637X, 9 p., p.1Article
CS and C34S observations of the NGC 7538 molecular cloudKAMEYA, O; HASEGAWA, T. I; HIRANO, N et al.Publications of the Astronomical Society of Japan. 1986, Vol 38, Num 6, pp 793-810, issn 0004-6264Article