NDLI: Distribution of dust in w31 complex

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Distribution of dust in w31 complex

Content Provider	NASA Technical Reports Server (NTRS)
Author	Verma, R. P. Rengarajan, T. N. Daniel, R. R. Tandon, S. N. Ghosh, Swarna Kanti Iyengar, K. V. K.
Copyright Year	1989
Description	W31 is a H II region/molecular cloud complex in the galactic plane at a distance of 6 Kpc. This complex consists of two prominent radio continuum sources (G10.2-0.3 and G10.3-0.1) representing H II regions. An extended region covering both these H II regions was mapped in the Far IR (FIR) using the TIFR 1 m balloon-borne telescope with an angular resolution of approx. 1 min and a dynamic range of 100. The resulting flux density distribution at an effective wavelength of 160 microns is presented. The coadded IRAS survey scan data at 60 and 100 microns were deconvolved using a maximum entropy method to generate the flux density maps of the same region. These 60 and 100 micron maps are given and are briefly discussed.
File Size	101943
Page Count	2
File Format	PDF
Alternate Webpage(s)	http://archive.org/details/NASA_NTRS_Archive_19910005631
Archival Resource Key	ark:/13960/t4fn62t0b
Language	English
Publisher Date	1989-12-01
Access Restriction	Open
Subject Keyword	Astrophysics Angular Resolution Infrared Sources Astronomy Molecular Clouds Infrared Astronomy Satellite Continuous Radiation Infrared Spectra Density Distribution Maximum Entropy Method Far Infrared Radiation Radio Emission Particle Flux Density Radiation Distribution Cosmic Dust Star Formation H Ii Regions Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science
Content Type	Text
Resource Type	Article

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