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| Query : 2017NewA...51..113D |
2017NewA...51..113D - New Astronomy, 51, 113-121 (2017)
The role of angular momentum transport in establishing the accretion rate-protostellar mass correlation.
DESOUZA A.L. and BASU S.
Journal keyword(s):
Simbad objects: 6
| Number of rows : 6 |
| 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 | NAME Taurus Complex | SFR | 04 41.0 | +25 52 | ~ | 4971 | 0 | |||||
| 2 | V* AB Aur | Ae* | 04 55 45.8458932216 | +30 33 04.292077032 | 7.20 | 7.16 | 7.05 | 6.96 | 6.70 | A0Ve | 1176 | 2 |
| 3 | NAME Orion Nebula Cluster | OpC | 05 35.0 | -05 29 | ~ | 2514 | 0 | |||||
| 4 | HD 100546 | Be* | 11 33 25.4408872296 | -70 11 41.241297948 | 6.71 | 6.30 | 6.64 | A0VaekB8_lB | 894 | 1 | ||
| 5 | HD 135344B | Or* | 15 15 48.4460065200 | -37 09 16.024369824 | 9.21 | 8.708 | F8V | 548 | 0 | |||
| 6 | NAME Ophiuchus Molecular Cloud | SFR | 16 28 06 | -24 32.5 | ~ | 3969 | 1 |
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