README web version of /home/usg/OPS/MTS/readme_xml/readme_78043800
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
The main goal of this proposal is to study four very young star clusters,
still associated to bright HII regions, in the Small Magellanic Cloud. The saudy
of the selected cluster will allow us to better investigate the role of massive
stars in the formation of low mass stars in low metallicity and low dust environments.
Two of the selected young clusters (NGC 371 and NGC 395-target of this section of
the proposal) are located NE to NGC 346. Many SNR are present in the region. Arcs
and filaments of HII seam to connect these three clusters, and they can be an example
of a SSPSF process.
Between NGC 346 and NGC 602 there is the HII complex N83-N84-N85. This complex hosts
two very young clusters: NGC 460 and NGC 456. The region appears as an outstanding
prototype of sequential start formation on a scale of 10^7 years in about 500 pc.
It contains several CO clouds, and expanding molecular shells coincident with either
the clusters and the SNRs. The shell of gas appear to be interacting with the nearby
molecular clouds, sweeping and compressing important mass of molecular hydrogen,
and perhaprs setting up a second generation of stars.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
ToO Information
ToO Activators List
Is this a Pre-imaging run ?
Pre-imaging Requirements
Source(s) of Pre-imaging
Pre-imaging sources not listed above
Do all your OBs comply with the instrument-specific requirements listed
on the instrument-specific Phase 2 web page ?
If this is a pre-imaging run, did you select PRE-IMAGING for the Observing
Category for each Observing Template ?
Do all your finding charts comply with both the general and instrument-specific
Phase 2 Web Pages ?
If you submitted OBs for standard stars, did you specify the magnitude
and spectral type of all standard stars in the OBs ?
Have you included OBs for any calibrations that you need but which are
not part of the Calibration Plan ?
If you are observing Moving Targets, have you attached suitable ephemeris
files to your OBs?
If you have preferences which OBs should be executed first, did you make
use of the User Priority field in the OBs ?
If this is a run that requires coordinated observations with other facilities,
did you give proper instructions in the Time-Critical Aspects Section ?
If you have prepared your finding charts with tools other than FIMS,
do they comply with the specifications on the FORS1 Phase 2 web page ?
Last creation of page: Tue Oct 6 15:40:16 2009
If you have comments, please contact usd-help@eso.org