output
19922026
most citedSkyrmion Lattice in a Chiral Magnet

4.8k citations

Showing 2010 · astro-ph.SRShow all

25 papers · 2 filters

astro-ph.SR2010★ 77 cited

An Interferometric Spectral-line Survey of IRC+10216 in the 345 GHz Band

Nimesh A. Patel, Ken H. Young, Carl A. Gottlieb +10

We report a spectral-line survey of the extreme carbon star IRC+10216 carried out between 293.9 and 354.8 GHz with the Submillimeter Array. A total of 442 lines were detected, more…

astro-ph.SR2010★ 14 cited

Submillimeter/millimeter observations of the molecular clouds associated with the Tycho' Supernova Remnant

Jin-Long Xu, Jun-Jie Wang, Martin Miller

We have carried out CO J=2-1 and CO J=3-2 observations toward Tycho's supernova remnant (SNR) using the KOSMA 3m-Telescope. From these observations we identified three molecular cl…

astro-ph.SR2010★ 30 cited

Star Formation Associated With the SNR IC443

Jin-Long Xu, Jun-Jie Wang, Martin Miller

We have performed the submillimeter and millimeter observations in CO lines toward supernova remnant (SNR) IC443. CO molecular shell is well coincident with the partial shell of th…

astro-ph.SR2010★ 9 cited

A study of three southern high-mass star-forming regions

C. Dedes, S. Leurini, F. Wyrowski +4

Based on color-selected IRAS point sources, we have started to conduct a survey of 47 high-mass star-forming regions in the southern hemisphere in 870um dust continuum and molecula…

astro-ph.SR2010★ 53 cited

Herschel-HIFI observations of high-J CO lines in the NGC 1333 low-mass star-forming region

U. A. Yıldız, E. F. van Dishoeck, L. E. Kristensen +60

Herschel-HIFI observations of high-J lines (up to J_u=10) of 12CO, 13CO and C18O are presented toward three deeply embedded low-mass protostars, NGC 1333 IRAS 2A, IRAS 4A, and IRAS…

astro-ph.SR2010★ 18 cited

HERSCHEL-HIFI spectroscopy of the intermediate mass protostar NGC7129 FIRS 2

D. Johnstone, M. Fich, C. McCoey +58

HERSCHEL-HIFI observations of water from the intermediate mass protostar NGC7129 FIRS 2 provide a powerful diagnostic of the physical conditions in this star formation environment.…