J/A+A/553/A87    Star forming regions in HST galaxies sample   (Drazinos+, 2013)

Star forming regions in a sample of HST spiral galaxies. Drazinos P., Kontizas E., Karampelas A., Kontizas M., Dapergolas A. <Astron. Astrophys., 553, A87-87 (2013)> =2013A&A...553A..87D 2013A&A...553A..87D
ADC_Keywords: Galaxy catalogs ; Morphology Keywords: methods: statistical - catalogs - galaxies: structure Abstract: The presence of small- and large-scale star formation structures in a sample of six spiral Hubble Space Telescope (HST) galaxies is investigated to identify small structures of young stars known as OB associations and to tell whether they are formed inside larger scale star forming stellar structures in a hierarchical form. This process was based on a friend-of-friend (FOF) algorithm applied to the bright, early type stars above a certain color cutoff limit in order to ensure that we include main sequence stars. A size criterion was introduced in order to apply the same algorithm to different types of stellar structures. Depending on their size, the structures were divided into the four categories of associations, aggregates, complexes, and supercomplexes. Star forming structures of the four types mentioned above are found in all six galaxies of our sample. The majority of the associations and aggregates (the smaller structures) found are lying inside larger structures like complexes and supercomplexes, indicating a hierarchical star formation mechanism. Description: The data used for our study were taken using HST/WFPC2 images and filters F555W(V) and F814W (I). They were retrieved from the HST data archive and were reduced using the HSTphot photometry package (Dolphin 2000, http://purcell.as.arizona.edu/hstphot/). A method based on a Friend of Friend algorithm were used to detect young stellar structures. In each catalogue we give for each structure, the position of the centre (deg), it's size (pc), the number of stars within the structure, and it's type as described in the relevant paper. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file ngc925.dat 42 775 NGC 925 young stellar structures ngc2541.dat 42 690 NGC 2541 young stellar structures ngc3351.dat 42 560 NGC 3351 young stellar structures ngc3621.dat 42 944 NGC 3621 young stellar structures ngc4548.dat 42 832 NGC 4548 young stellar structures ngc5457.dat 42 710 NGC 5457 young stellar structures -------------------------------------------------------------------------------- Byte-by-byte Description of file: ngc*.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 -- Index Sequential number within the Group 5- 14 F10.6 deg RAdeg Right ascension (J2000) 16- 25 F10.6 deg DEdeg Declination (J2000) 27- 30 I4 -- Nstars Number of stars in Group 32- 40 F9.3 pc Size Group size (parsec) 42 I1 -- Type [1/4] Type of Group: 1=Association, 2=Aggregate, 3=Complex, 4=Supercomplex -------------------------------------------------------------------------------- Acknowledgements: Petros Drazinos, pdrazinos(at)noa.gr
(End) Petros Drazinos [UOA, Greece], Patricia Vannier [CDS] 18-Feb-2014
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line