Citation: Dl. Lambert et al., Infrared Space Observatory spectra of R Coronae Borealis stars. I. Emission features in the interval 3-25 microns, ASTROPHYS J, 555(2), 2001, pp. 925-931
Authors:
Ivans, II
Kraft, RP
Sneden, C
Smith, GH
Rich, RM
Shetrone, M
Citation: Ii. Ivans et al., New analyses of star-to-star abundance variations among bright giants in the mildly metal-poor globular cluster M5, ASTRONOM J, 122(3), 2001, pp. 1438-1463
Authors:
Sneden, C
Cowan, JJ
Ivans, II
Fuller, GM
Burles, S
Beers, TC
Lawler, JE
Citation: C. Sneden et al., Evidence of multiple r-process sites in the early galaxy: New observationsof CS 22892-052, ASTROPHYS J, 533(2), 2000, pp. L139-L142
Authors:
Clementini, G
Di Tomaso, S
Di Fabrizio, L
Bragaglia, A
Merighi, R
Tosi, M
Carretta, E
Gratton, RG
Ivans, II
Kinard, A
Marconi, M
Smith, HA
Wilhelm, R
Woodruff, T
Sneden, C
Citation: G. Clementini et al., CU Comae: A new field double-mode RR Lyrae variable the most metal-poor discovered to date, ASTRONOM J, 120(4), 2000, pp. 2054-2064
Citation: Ii. Ivans et al., The mildly metal-poor globular cluster M4: Star-to-star abundance variations in 20 giants, ASTRO SP SC, 265(1-4), 1999, pp. 195-196
Authors:
Ivans, II
Sneden, C
Kraft, RP
Suntzeff, NB
Smith, VV
Langer, GE
Fulbright, JP
Citation: Ii. Ivans et al., Star-to-star abundance variations among bright giants in the mildly metal-poor globular cluster M4, ASTRONOM J, 118(3), 1999, pp. 1273-1300