On the Identification of High‐Mass Star Forming Regions Using<i>IRAS</i>: Contamination by Low‐Mass Protostars

Tyler L. Bourke(University of Manchester), G. Robinson(UNSW Sydney), A. R. Hyland(UNSW Sydney)
The Astrophysical Journal
May 27, 2005
10.1086/429818
Cited by 27

Related Papers

Advancing Astrophysics with the Square Kilometre Array
|Unknown|2015|836
From Molecular Cores to Planet‐forming Disks: An<i>SIRTF</i>Legacy Program
|Publications of the Astronomical Society of the Pacific|2003|546
Advancing Astrophysics with the Square Kilometre Array (AASKA14)
|Unknown|2015|513
The ALMA Protostellar Interferometric Line Survey (PILS)
|Astronomy and Astrophysics|2016|401
The spatial distribution of star formation in the solar neighbourhood: do all stars form in dense clusters?
|Monthly Notices of the Royal Astronomical Society Letters|2010|346