Orion Proplyds and The Eagle's Eggs
- 1 January 1997
- journal article
- Published by Cambridge University Press (CUP) in Symposium - International Astronomical Union
- Vol. 182, 551-560
- https://doi.org/10.1017/s0074180900061945
Abstract
We describe the effects of environment on low-mass star formation, from the perspective that most stars in the galaxy form in dense clusters and aggregates in GMCs, often in the presence of massive OB stars. First, we discuss the observational evidence for circumstellar disks around stars of the Trapezium Cluster, and how they are affected by their environment. Second, we examine the more distant M 16, where photo-evaporation by OB stars may disrupt the star formation process, and may inhibit the development of circumstellar disks.Keywords
This publication has 22 references indexed in Scilit:
- Circumstellar disks in the Trapezium ClusterPublished by Springer Nature ,2006
- A Search for Thermal Infrared Emission from Three Silhouette Disks in OrionThe Astronomical Journal, 1997
- A Two-Wind Interaction Model for ProplydsThe Astrophysical Journal, 1996
- Encounters with Protostellar Disks. II. Disruption and Binary FormationThe Astrophysical Journal, 1995
- Constraints on Circumstellar Disk Masses in the Trapezium ClusterThe Astrophysical Journal, 1995
- Additional constraints on circumstellar disks in the Trapezium ClusterThe Astronomical Journal, 1994
- HST photometry of the trapezium clusterThe Astrophysical Journal, 1994
- Infrared luminosity functions for the young stellar population associated with the L1641 molecular cloudThe Astrophysical Journal, 1993
- On the spatial distribution of pre-main-sequence stars in TaurusThe Astronomical Journal, 1993
- The Trapezium cluster of the Orion nebulaThe Astrophysical Journal, 1986