J/other/ChA+A/28.308     JHK' photometry in GGD 12-15 region     (Fang+, 2004)

Near infrared observations of the star formation region GGD 12-15. Fang M., Yao Y.-Q. <Chinese Astron., 28, 308-322 (2004)> =2004ChA&A..28..308F 2004ChA&A..28..308F
ADC_Keywords: Clusters, open ; Photometry, infrared Keywords: infrared: stars - Galaxy: open clusters and associations: GGD1215 - stars: formation Abstract: Near infrared imaging observations in JHK broad bands and H2 v=1-0 S(1) narrow band of the star formation region GGD12-15 are presented in this article. The images reveal young compact infrared clusters and infrared nebulae in association with infrared sources, as well as outflow activities characterized by H2 emission knots. Most of the infrared point sources are invisible in the optical wave band. The JHK' photometric results of 76 infrared point sources contain 32 with infrared excess, and 5 with the characteristics of protostars, indicating very active star formation activities in the molecular clouds. Description: GGD12-15 was observed with the 1.88-m telescope and OASIS infrared camera of Institute of Astrophysics of Okayama in Japan on 1999 November 2. Objects: ------------------------------------------------------------- RA (2000) DE Designation(s) ------------------------------------------------------------- 06 10 51.0 -06 11 54 GGD 12-15 = [BDB2003] G213.88-11.83 ------------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 29 76 Photometric results of infrared point sources in the GGD12-15 region table2.dat 25 30 The deeply-embedded infrared point sources in the GGD12-15 region table3.dat 25 14 The H2 molecular line emission knots in the GGD12-15 region -------------------------------------------------------------------------------- Byte-by-byte Description of file: table[12].dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- NIRS Sequential number (1) 4- 9 F6.1 arcsec DRA Offset in right ascension (G1) 11- 16 F6.1 arcsec DDE Offset in declination (G1) 18- 21 F4.1 mag K'mag K' magnitude 23- 25 F3.1 mag H-K' ?=- H-K' colour index 27- 29 F3.1 mag J-H ? J-H colour index -------------------------------------------------------------------------------- Note (1): Table1: [FY2004] NIRS NN in Simbad Table2: [FY2004] NIRSe NN in Simbad -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- H2 H2 knot sequential number, [FY2004] H2 NN in Simbad 4- 8 F5.1 arcsec DRA Offset in right ascension (G1) 10- 14 F5.1 arcsec DDE Offset in declination (G1) 16- 19 F4.1 10-16W/m2/um Fv1-0 Flux in H2 v=1-0 S(1) band (2.12µm) 21- 23 F3.1 arcsec Aper Aperture used in measurement of the hydrogen molecular emission 25 A1 --- Conf [EK] Configuration (1) -------------------------------------------------------------------------------- Note (1): Configuration as follows: K = H2 knot E = elongation -------------------------------------------------------------------------------- Global notes Note (G1): The origin of the offset is the position of NIRS3 RA = 06 08 23.72, DE=-06 11 13.8, B1950 -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 24-Aug-2005
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