README web version of /home/usg/OPS/MTS/readme_xml/readme_83018100
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
We have discovered high-mass protostellar candidates in M17 whose SEDs
yield luminosities between 100 and several 1000 L_sol. Their colors and J,K-band
spectroscopy suggest temperatures of 3000 to 7000 K. All sources show the 2.3 mu
CO band head feature in absorption, indicating ongoing accretion. These properties
are in accord with theoretical models of extremely young (~ 10^4 yr), heavily accreting
(10^-5 - 10^-3 M_sol/yr) protostars currently developing into high-mass stars.
We wish to confirm our estimates of the effective temperature and corroborate the
ongoing accretion activity of these protostars by optical spectroscopy centered
on the Halpha line.
The results from the spectra will reveal the nature of the sources by placing them
unambiguously onto recent evolutionary tracks. If true, these objects will be in
a rare evolutionary stage supporting the high mass-accretion rate and represent
the rare missing link between luminous high-mass cores and ultra-compact HII regions.
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 15:40:29 2009
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