Other
Scientific paper
Jan 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ycat..33550651f&link_type=abstract
VizieR On-line Data Catalog: J/A+A/355/651. Originally published in: 2000A&A...355..651F
Other
Clusters: Open, Stars: Pre-Main Sequence, X-Ray Sources
Scientific paper
We analyze six ROSAT HRI observations pointed toward the Star Forming Region (SFR) NGC 2264. Three are pointed to the southern star formation core, the other three about 20' to the north. We detect 169 X-ray sources, ~95% of which are likely to be Pre Main Sequence (PMS) stars, significantly enlarging the known population of the SFR in the area covered by the observations. Using published BVRI photometry we place the X-ray sources with well defined optical counterparts on the HRI diagram and estimate their masses and ages. Our comparison of the mass function and age distribution of the X-ray sources with results previously obtained for NGC 2264, demonstrates that deep X-ray observations provide, at least in this case, a very efficient method of selecting SFR members and does not introduce stronger biases than other methods.
(2 data files).
Damiani Ferruccio
Favata Fabio
Flaccomio Ettore
Harnden Frank R. Jr.
Micela Giuseppina
No associations
LandOfFree
HRI observations of PMS stars in NGC 2264 (Flaccomio+, 2000) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with HRI observations of PMS stars in NGC 2264 (Flaccomio+, 2000), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and HRI observations of PMS stars in NGC 2264 (Flaccomio+, 2000) will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1690203