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2020ApJ...889...63H - Astrophys. J., 889, 63-63 (2020/January-3)
Metallicity and α-element abundance gradients along the Sagittarius stream as seen by APOGEE.
HAYES C.R., MAJEWSKI S.R., HASSELQUIST S., ANGUIANO B., SHETRONE M., LAW D.R., SCHIAVON R.P., CUNHA K., SMITH V.V., BEATON R.L., PRICE-WHELAN A.M., ALLENDE PRIETO C., BATTAGLIA G., BIZYAEV D., BROWNSTEIN J.R., COHEN R.E., FRINCHABOY P.M., GARCIA-HERNANDEZ D.A., LACERNA I., LANE R.R., MESZAROS S., MONI BIDIN C., MUNOZ R.R., NIDEVER D.L., ORAVETZ A., ORAVETZ D., PAN K., ROMAN-LOPES A., SOBECK J. and STRINGFELLOW G.
Abstract (from CDS):
Abstract Copyright: © 2020. The American Astronomical Society. All rights reserved.
Journal keyword(s): Sagittarius dwarf spheroidal galaxy - Milky Way stellar halo - Chemical abundances - Galaxy evolution - Tidal tails - Galaxy chemical evolution - Galaxy abundances - Stellar kinematics - Stellar abundances - Dwarf galaxies
VizieR on-line data: <Available at CDS (J/ApJ/889/63): table1.dat>
Simbad objects: 884
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