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2019ApJ...878..110F - Astrophys. J., 878, 110-110 (2019/June-3)
Relative alignment between the magnetic field and molecular gas structure in the Vela C giant molecular cloud using low- and high-density tracers.
FISSEL L.M., ADE P.A.R., ANGILE F.E., ASHTON P., BENTON S.J., CHEN C.-Y., CUNNINGHAM M., DEVLIN M.J., DOBER B., FRIESEN R., FUKUI Y., GALITZKI N., GANDILO N.N., GOODMAN A., GREEN C.-E., JONES P., KLEIN J., KING P., KOROTKOV A.L., LI Z.-Y., LOWE V., MARTIN P.G., MATTHEWS T.G., MONCELSI L., NAKAMURA F., NETTERFIELD C.B., NEWMARK A., NOVAK G., PASCALE E., POIDEVIN F., SANTOS F.P., SAVINI G., SCOTT D., SHARIFF J.A., SOLER J.D., THOMAS N.E., TUCKER C.E., TUCKER G.S., WARD-THOMPSON D. and ZUCKER C.
Abstract (from CDS):
Abstract Copyright: © 2019. The American Astronomical Society. All rights reserved.
Journal keyword(s): dust, extinction - ISM: individual objects: Vela C - ISM: magnetic fields - ISM: molecules - molecular data
Simbad objects: 8
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