2004BaltA..13..357B

Query : 2004BaltA..13..357B

2004BaltA..13..357B - Baltic Astronomy, 13, 357-364 (2004/August-0)

Dynamical and radiation processes in star and planet formation.

BALLY J.

Abstract (from CDS):

Most stars are born in dense environments where radiation fields and dynamical interactions with sibling stars may profoundly influence the ultimate outcome of star formation. I review how radiation fields photo-evaporate cloud cores and circumstellar disks. I also comment on the role of gravitational interactions with sibling stars. These processes may be fundamental for determining the initial mass function of stars and pose hazards to planet formation.

Abstract Copyright: ∼

Journal keyword(s): ISM: prestellar clouds - stars: formation, circumstellar disks, jets

Simbad objects: 14

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Number of rows : 14
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 Ass Per OB 1 As* 02 21 +57.6           ~ 174 1
2 HH 498 HH 03 28 52.2 +31 22 45           ~ 5 0
3 NGC 1333 OpC 03 29 11.3 +31 18 36           ~ 1450 1
4 HH 243 HH 05 32 27.83 +12 53 14.6   17.0       ~ 117 0
5 NAME Orion Nebula Cluster OpC 05 35.0 -05 29           ~ 2330 0
6 V* LL Ori Or* 05 35 05.6361678504 -05 25 19.520320800 12.997 12.309 11.517   10.034 K0-K3e 108 1
7 M 42 HII 05 35 17 -05 23.4           ~ 4073 0
8 NAME Ori A MoC 05 38 -07.1           ~ 3008 0
9 NAME Upper Sco-Cen As* 16 15 -24.2           ~ 1330 1
10 IRAS 20126+4104 Y*O 20 14 25.8816769656 +41 13 36.879427236           B2.5-B0.5 440 0
11 HH 200 HH 20 57 +77.6           ~ 16 0
12 IRAS 20582+7724 Y*O 20 57 12.9250225656 +77 35 43.656301932           ~ 117 0
13 LDN 1228 DNe 20 57 13 +77 35.8           ~ 128 0
14 HH 499 HH ~ ~           ~ 5 0

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