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| Query : 2018MNRAS.480.4754G |
2018MNRAS.480.4754G - Mon. Not. R. Astron. Soc., 480, 4754-4760 (2018/November-2)
Calculated oscillator strengths for the strongest lines of cosmochronological interest in the visible spectrum of singly ionized uranium (U II).
GAMRATH S., PALMERI P. and QUINET P.
Abstract (from CDS):
Abstract Copyright: © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): atomic data - atomic processes
Simbad objects: 1
| Number of rows : 1 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | BD-16 251 | RG* | 01 29 31.1311443552 | -16 00 45.495314460 | 12.527 | 12.427 | 11.642 | 11.189 | 10.713 | CEMP | 318 | 0 |
| Query : 2018MNRAS.480.4754G |
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Hierarchy :
number of linked objects
whatever the membership probability is (see description here ) :
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BD-16 251
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RAVE J012931.1-160046
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TYC 5852-1248-1
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Gaia DR1 2451773937663757696
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| BPS CS 31082-0001 | SMSS J012931.13-160045.7 |
Gaia DR2 2451773941958712192
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2MASS J01293113-1600454
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TIC 257422252 |
Gaia DR3 2451773941958712192
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References (318 between 1850 and 2026) (Total 318)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system). |
Link by name to the catalogue in VizieR :
| BD-16 251 | 2MASS J01293113-1600454 | RAVE J012931.1-160046 | TYC 5852-1248-1 | Gaia DR2 2451773941958712192 |
| Gaia DR3 2451773941958712192 | Gaia DR1 2451773937663757696 |
Search by coordinates in Vizier (radius: 5 arcsec)
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