Table 3
Observationally determined distances of RS Pup (“IRSB” stands for “infrared surface brightness”).
| Distance [pc] | Method | p-factor | Source |
|
|
|||
| 1 780 ± 200 | Light echoes | − | H72 |
| 2 580 ± 300 | IRSB | 1.341 | G93 |
| 2 040 | Hipparcos | − | P97 |
| 1 930 | ZAMS | − | DB97 |
|
IRSB | 1.341 | F03 |
|
IRSB | 1.341 | S04 |
| 1 800 ± 130 | IRSB | 1.341 | T03 |
| 1 706 ± 228 | IRSB (Bayesian) | 1.341 | B03 |
| 2 004 ± 59 | IRSB (least squares) | 1.341 | B05 |
| 1 984 ± 122 | IRSB (Bayesian) | 1.341 | B05 |
|
Hipparcos | − | VL07a |
|
Hipparcos | − | VL07b |
|
IRSB | 1.341 | F07 |
| 1 765 ± 34 ± 65 | BW | 1.272 | G08 |
| 1 810 ± 30 | IRSB | 1.249 | S11 |
| 1 568 ± 30 ± 72 | BW | 1.112 | G13 |
|
|
|||
| 1910 ± 80 | Echoes (MW dust) | − | K14 |
| 1940 ± 70 | Echoes (Rayleigh) | − | K14 |
Notes. B03: Barnes et al. (2003); B05: Barnes et al. (2005); DB97: Di Benedetto (1997); P97: Perryman & ESA (1997); F03: Fouqué et al. (2003); F07: Fouqué et al. (2007); G08: Groenewegen (2008); G13: Groenewegen (2013); G93: Gieren et al. (1993); H72: Havlen (1972); K14: present work; S04: Storm et al. (2004); S11: Storm et al. (2011); T03: Tammann et al. (2003); VL07a: van Leeuwen (2007); VL07b: van Leeuwen et al. (2007).
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