T. Kuwahara

发表

, CO, AND PLANCK/IRAS DUST PROPERTIES IN THE HIGH LATITUDE CLOUD COMPLEX, MBM 53, 54, 55 AND HLCG 92 − 35. POSSIBLE EVIDENCE FOR AN OPTICALLY THICK ENVELOPE AROUND THE CO CLOUDS

J. Dickey, T. Hayakawa, Y. Fukui, 2014, 1401.7398.

A DETAILED STUDY OF NON-THERMAL X-RAY PROPERTIES AND INTERSTELLAR GAS TOWARD THE γ-RAY SUPERNOVA REMNANT RX J1713.7−3946

T. Tanaka, A. Kawamura, Tsuyoshi Inoue, 2014, 1401.7418.

NON-THERMAL X-RAYS AND INTERSTELLAR GAS TOWARD THE γ-RAY SUPERNOVA REMNANT RX J1713.7−3946: EVIDENCE FOR X-RAY ENHANCEMENT AROUND CO AND H i CLUMPS

H. Yamamoto, T. Tanaka, A. Kawamura, 2013, 1304.7722.

Interstellar Gas and X-rays toward the Young Supernova Remnant RCW 86; Pursuit of the Origin of the Thermal and Non-Thermal X-ray

H. Yamamoto, E. Reynoso, Y. Fukui, 2016, 1606.07745.

MOLECULAR CLOUDS TOWARD THE SUPER STAR CLUSTER NGC 3603; POSSIBLE EVIDENCE FOR A CLOUD–CLOUD COLLISION IN TRIGGERING THE CLUSTER FORMATION

H. Maezawa, A. Kawamura, T. Hayakawa, 2013, 1306.2090.

Ground-based millimeter-wave observation of stratospheric ClO over Atacama, Chile in the mid-latitude Southern Hemisphere

H. Maezawa, Y. Fukui, T. Okuda, 2012 .

Ground-based millimeter-wave observations of water vapor emission (183 GHz) at Atacama, Chile

S. Asayama, H. Maezawa, Y. Fukui, 2008 .