A dataset provided by the European Space Agency

Name STARLESS
Title ARE STARLESS BOK GLOBULES REALLY DEVOID OF STARS? ISOCAM IMAGING OF STARLESS BOK GLOBULES
URL

http://nida.esac.esa.int/nida-sl-tap/data?RETRIEVAL_TYPE=OBSERVATION&PRODUCT_LEVEL=ALL&obsno=106001130

DOI https://doi.org/10.5270/esa-xhprv9u
Author Dan P. Clemens
Description bok globules are the smallest and simplest molecular clouds capable of forming new stars. past work using the iras data base has helped to identify samples of nearby globules with infrared signatures of current embedded star formation. perhaps equally important, iras data have been used to identify bok globules which appear to not have embedded star formation. subsequent studies of this starless sample of globules have been initiated, with the goal of characterizing the physical conditions of these simple clouds before stars have formed. however, iras was not able to detect all low mass stars, and the quality of the starless sample of bok globules is unknown, if not suspect. using iso with the isocam instrument, we propose to conduct a very deep search for stars in the starless globule sample. the detection limit is set so that any hydrogen burning star or any yso will be clearly identified within the globule cores and very near envelopes. the results of such a search will be analyzed in order to: 1) establish a bona fide sample of truly starless bok globules; 2) determine the star formation rates and efficiencies for stars in the 0.08 - 0.7 solar mass range (fainter than iras, but detectable by iso) for the globules here found to contain low-mass stars; and 3) test for low-mass stellar clustering in bok globules to see if such clustering is universal in star forming regions. this survey will be conducted using the isocam instrument in the lw2 (6.75 micron) and lw3 (15 micron) filters in a micro-stepping map mode to return maps of 3 arcsecond resolution (pfov) over areas of 3.7 x 3.7 arcmin square.
Instrument CAM01 , PHT03
Temporal Coverage 1996-02-26T05:53:34Z/1998-03-16T16:32:37Z
Version 1.0
Mission Description The Infrared Space Observatory (ISO) was the worlds first true orbiting infrared observatory. Equipped with four highly-sophisticated and versatile scientific instruments, it was launched by Ariane in November 1995 and provided astronomers world-wide with a facility of unprecedented sensitivity and capabilities for a detailed exploration of the Universe at infrared wavelengths.
Creator Contact https://support.cosmos.esa.int/iso/
Date Published 1999-04-09T00:00:00Z
Keywords ISO, infrared, SWS, LWS, ISOCAM, ISOPHOT
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dan P. Clemens, 1999, 'ARE STARLESS BOK GLOBULES REALLY DEVOID OF STARSquestionMark ISOCAM IMAGING OF STARLESS BOK GLOBULES', 1.0, European Space Agency, https://doi.org/10.5270/esa-xhprv9u