From Molecular Cores to Planet-forming Disks with SIRTF

Details From Molecular Cores to Planet-forming Disks with SIRTF From Molecular Cores to Planet-forming Disks with SIRTF

2003-10-28

arxiv.org/abs/astro-ph/0310811v1

Astronomy and Astrophysics

Astrophysics

6 pages, from Fourth Cologne-Bonn-Zermatt-Symposium, The Dense Interstellar Matter in Galaxies

Scientific paper

The SIRTF mission and the Legacy programs will provide coherent data bases for extra-galactic and Galactic science that will rapidly become available to researchers through a public archive. The capabilities of SIRTF and the six legacy programs are described briefly. Then the cores to disks (c2d) program is described in more detail. The c2d program will use all three SIRTF instruments (IRAC, MIPS, and IRS) to observe sources from molecular cores to protoplanetary disks, with a wide range of cloud masses, stellar masses, and star-forming environments. The SIRTF data will stimulate many follow-up studies, both with SIRTF and with other instruments.

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