Details on Acronym: [TTW2011] | |
| [TTW2011] | (Tumlinson+Thom+Werk+, 2011) |
| Write: | <<[TTW2011] SDSS JHHMM+DDMM NNN-NNN>> <<[TTW2011] JHHMM+DDMM NNN_NNN>> (not recognised by Simbad, but found in literature) |
| N: | 30+12+26 |
| Object: | G (SIMBAD class: Galaxy) |
| Note: | HST COS observations. The galaxies are labeled with two numbers: the position angle from the QSO (N through E), and the angular separation in arcseconds. |
| Ref: | =2011Sci...334..948T |
| by | TUMLINSON J. , THOM C., WERK J.K., PROCHASKA J.X., TRIPP T.M., WEINBERG D.H., PEEPLES M.S., O'MEARA J.M., OPPENHEIMER B.D., MEIRING J.D., KATZ N.S., DAVE R., FORD A.B., SEMBACH K.R. |
| Sci, 334, 948-952 (2011) | |
| The large, oxygen-rich halos of star-forming galaxies are a major reservoir of Galactic metals. | |
| o | Tables S1-S2: <[TTW2011] SDSS JHHMM+DDMM NNN-NNN> N=30+12. |
| Ref: | =2012ApJS..198....3W |
| by | WERK J.K. , PROCHASKA J.X., THOM C., TUMLINSON J., TRIPP T.M., O'MEARA J.M., MEIRING J.D. |
| Astrophys. J., Suppl. Ser., 198, 3 (2012) | |
| The COS-Halos survey: Keck LRIS and Magellan MagE optical spectroscopy. | |
| o | Tables 2, 4-5: <[TTW2011] SDSS JHHMM+DDMM NNN-NNN> N=26 added. |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |