J/ApJ/629/288       Infrared sources near AFGL 5142          (Chen+, 2005)

Near-infrared imaging of the star formation region AFGL 5142. Chen Y., Yao Y., Yang J., Zeng Q., Sato S. <Astrophys. J., 629, 288-298 (2005)> =2005ApJ...629..288C 2005ApJ...629..288C
ADC_Keywords: Associations, stellar ; Infrared sources Keywords: ISM: individual (AFGL 5142) - ISM: jets and outflows - ISM: lines and bands - open clusters and associations: general Abstract: Near-infrared JHK' and H2 v=1-0 S(1) imaging observations of the star-forming region AFGL 5142 are presented. A cluster of young stars is confirmed to be embedded in the dense molecular cloud core. Many point sources are newly detected. The cluster's K'-magnitude distribution and [H-K'] color peak have brighter and redder magnitudes than those outside the cluster. Many of the cluster sources exhibit infrared excesses typical of T Tauri stars, Herbig Ae/Be stars, and protostars. The observations also reveal new H2 line emission around the cluster, exhibiting several jets, filaments, and a faint elliptical structure. The jets are associated with the CO outflows in the region. The powering sources of the jets, the CO outflows, and the small faint elliptical structure are identified and analyzed individually. The strong H2 jets and faint diffuse emission further confirm that the cluster is in an early stage of evolution. Description: Under photometric conditions, images of AFGL 5142 were taken with Okayama Astrophysical System for Infrared Imaging and Spectroscopy at the 1.88m telescope at Okayama Astronomical Observatory in Japan in 1997 October, 1999 November, and 2000 November. Objects: ----------------------------------------------- RA (2000) DE Designation(s) ----------------------------------------------- 05 30 45.9 +33 47 56 AFGL 5142 = RAFGL 5142 ----------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 38 164 Near-Infrared Photometry of AFGL 5142 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Seq Sequential number, [CYY2005] NIRS NNN in Simbad 4 A1 --- n_Seq [cd] Note on Seq (1) 6- 12 F7.2 arcsec DRA Offset in right ascension (2) 13- 18 F6.1 arcsec DDE Offset in declination (2) 20- 24 F5.2 mag K'mag K' magnitude 26- 30 F5.2 mag [H-K'] ?=- [H-K'] colour index 32- 35 F4.2 mag [J-H] ?=- [J-H] colour index 37- 38 I2 --- [HTT95] ?=- Number given to the point source in Table 2 of Hunter et al., (1995A&A...302..249H 1995A&A...302..249H), [HTT95] IR NN in Simbad -------------------------------------------------------------------------------- Note (1): c = IRS 1 (Hunter et al., 1995A&A...302..249H 1995A&A...302..249H), [HTT95] IRS 1 d = IRS 2 (Hunter et al., 1995A&A...302..249H 1995A&A...302..249H), [HTT95] IRS 2 Note (2): DRA and DDE offsets from NIRS 30 at 05:30:46.04+33:47:54.7 (J2000.0) in POSS. -------------------------------------------------------------------------------- History: * 25-Aug-2006: From electronic version of the journal * 28-Sep-2006: For [CYY2005] NIRS 1, [HTT95] 55 corrected into [HTT95] 19 ([HTT95] IRS 1 = [HTT95] 19 in Simbad)
(End) Patricia Vannier [CDS] 25-Aug-2006
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