155 citations · 4k across the 119 of their papers we have counts for
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First sub-arcsecond submillimeter-wave [C I] image of 49 Ceti with ALMA
Aya E. Higuchi, Kazuya Saigo, Hiroshi Kobayashi +7
We present the first sub-arcsecond images of 49 Ceti in the [C I]3P1-3P0 emission and the 614 micron dust continuum emission observed with ALMA, as well as that in the CO(J=3-2) em…
Sulfur-Bearing Species Tracing the Disk/Envelope System in the Class I Protostellar Source Elias 29
Yoko Oya, Ana López-Sepulcre, Nami Sakai +11
We have observed the Class I protostellar source Elias 29 with Atacama Large Millimeter/submillimeter Array (ALMA). We have detected CS, SO, SO, SO, and SiO line emissio…
Physical and chemical fingerprint of protostellar disc formation
E. Artur de la Villarmois, J. K. Jørgensen, L. E. Kristensen +5
(Abridged) The purpose of this paper is to explore and compare the physical and chemical structure of Class I low-mass protostellar sources on protoplanetary disc scales. We presen…
A 3 mm Spectral Line Survey toward the Barred Spiral Galaxy NGC 3627
Yoshimasa Watanabe, Yuri Nishimura, Kazuo Sorai +3
We conduct spectral line survey observations in the 3 mm band toward a spiral arm, a bar-end, and a nuclear region of the nearby barred spiral galaxy NGC 3627 with the IRAM 30 m te…
The Effect of Far-infrared Radiation on the Hyperfine Anomaly of the OH 18 cm Transition
Yuji Ebisawa, Nami Sakai, Karl M. Menten +1
We present observations of the four hyperfine structure components of the OH 18 cm transition (1612, 1665, 1667 and 1720 MHz) toward Heiles Cloud 2 (HCL2) in Taurus and the dense c…
An unbiased spectral line survey observation toward the low-mass star-forming region L1527
Kento Yoshida, Nami Sakai, Yuri Nishimura +5
An unbiased spectral line survey toward a solar-type Class 0/I protostar, IRAS04368+2557, in L1527 has been carried out in the 3 mm band with the Nobeyama 45 m telescope. L1527 is…