M. Saito

activity

20042024

μ

m dark High-mass clumps in Early Stages (ASHES). I. Pilot Survey: Clump Fragmentation

207 citations · 3.8k across the 104 of their papers we have counts for

collaborators

Showing 2014 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2014★ 25 cited

Discovery of Star Formation in the Extreme Outer Galaxy Possibly Induced by a High-velocity Cloud Impact

Natsuko Izumi, Naoto Kobayashi, Chikako Yasui +3

We report the discovery of star formation activity in perhaps the most distant molecular cloud in the extreme outer galaxy. We performed deep near infrared imaging with the Subaru…

astro-ph.GA2014★ 194 cited

Formation of a Keplerian disk in the infalling envelope around L1527 IRS: transformation from infalling motions to Kepler motions

Nagayoshi Ohashi, Kazuya Saigo, Yusuke Aso +9

We report Atacama Large Millimeter/submillimeter Array (ALMA) cycle 0 observations of C $^{18}$ O ( $J = 2 - 1$ ), SO ( $J_{N} = 6_{5} - 5_{4}$ ) and 1.3mm dust continuum toward L1527 IRS, a class 0…

astro-ph.GA2014★ 84 cited

High abundance ratio of $^{13}$ CO to C $^{18}$ O toward photon-dominated regions in the Orion-A giant molecular cloud

Yoshito Shimajiri, Yoshimi Kitamura, Masao Saito +11

Aims. We derive physical properties such as the optical depths and the column densities of $^{13}$ CO and C $^{18}$ O to investigate the relationship between the far ultraviolet (FUV)…

Discovery of Star Formation in the Extreme Outer Galaxy Possibly Induced by a High-velocity Cloud Impact

Formation of a Keplerian disk in the infalling envelope around L1527 IRS: transformation from infalling motions to Kepler motions

High abundance ratio of 13CO to C18O toward photon-dominated regions in the Orion-A giant molecular cloud

High abundance ratio of $^{13}$ CO to C $^{18}$ O toward photon-dominated regions in the Orion-A giant molecular cloud