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Query : 2000ApJ...538..226V |
2000ApJ...538..226V - Astrophys. J., 538, 226-232 (2000/July-3)
Interstellar clump behavior and magnetic effects in small clumps.
VALLEE J.P.
Abstract (from CDS):
These exponent values differ from those found by Larson for molecular clouds with sizes greater than 1 pc. These differences in c and k could be indicative of ongoing accretion processes in shocked media as a prelude to star formation. The energy distribution in clumps reveals the following: the support against gravitational collapse in clumps with sizes greater than 0.1 pc comes mainly from turbulent energy, while smaller clumps with sizes less than 0.1 pc are supported by both magnetic and turbulent energies. The clump size of 0.1 pc is critical in many other respects.
Abstract Copyright: ∼
Journal keyword(s): ISM: Dust, Extinction - Infrared: ISM: Continuum - ISM: Clouds - ISM: Magnetic Fields - Stars: Formation
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 | LBN 119.83-06.05 | MoC | 00 28 43.5075 | +56 41 56.868 | ~ | 69 | 0 | |||||
2 | [CB88] 34 | MoC | 05 47 02.3 | +21 00 10 | ~ | 61 | 0 | |||||
3 | [CB88] 54 | MoC | 07 04 21.2170 | -16 23 15.000 | ~ | 48 | 0 | |||||
4 | LDN 146 | MoC | 16 57 17.5 | -16 09 18 | ~ | 77 | 1 | |||||
5 | LDN 1177 | DNe | 21 17 38.62 | +68 17 34.0 | ~ | 88 | 1 |
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