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Query : 2013A&A...549A.112M |
2013A&A...549A.112M - Astronomy and Astrophysics, volume 549A, 112-112 (2013/1-1)
Why circumstellar disks are so faint in scattered light: the case of HD 100546.
MULDERS G.D., MIN M., DOMINIK C., DEBES J.H. and SCHNEIDER G.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): scattering - radiative transfer - circumstellar matter - stars: individual: HD 100546 - protoplanetary disks
Simbad objects: 5
Number of rows : 5 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | V* GG Tau | Or* | 04 32 30.3506925552 | +17 31 40.494063144 | 14.84 | 14.78 | 13.40 | 11.54 | M0e+M2.0e | 736 | 1 | |
2 | HD 100546 | Be* | 11 33 25.4408872296 | -70 11 41.241297948 | 6.71 | 6.30 | 6.64 | A0VaekB8_lB | 806 | 1 | ||
3 | HD 106797 | Pu* | 12 17 06.3097594320 | -65 41 34.654744752 | 6.073 | 6.054 | A0V | 56 | 0 | |||
4 | HD 109200 | PM* | 12 33 31.3825438408 | -68 45 20.912700882 | 8.472 | 7.987 | 7.140 | 6.661 | 6.237 | K1V | 130 | 0 |
5 | HD 141569 | Y*O | 15 49 57.7482550392 | -03 55 16.341617064 | 7.22 | 7.20 | 7.12 | 7.00 | 7.04 | A2VekB9mB9(_lB) | 540 | 0 |
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