J/MNRAS/387/954     H2 imaging of NGC 1333, L1455, L1448 and B1   (Davis+, 2008)

A shallow though extensive H22.122-µm imaging survey of Taurus-Auriga-Perseus. I. NGC 1333, L1455, L1448 and B1. Davis C.J., Scholz P., Lucas P., Smith M.D., Adamson A. <Mon. Not. R. Astron. Soc., 387, 954-968 (2008)> =2008MNRAS.387..954D 2008MNRAS.387..954D
ADC_Keywords: Associations, stellar ; Infrared sources ; Interstellar medium Keywords: stars: formation - ISM: individual: Perseus - ISM: jets and outflows - ISM: kinematics and dynamics - infrared: stars Abstract: We discuss wide-field near-infrared (near-IR) imaging of the NGC 1333, L1448, L1455 and B1 star-forming regions in Perseus. The observations have been extracted from a much larger narrow-band imaging survey of the Taurus-Auriga-Perseus complex. These H2 2.122um observations are complemented by broad-band K imaging, mid-IR imaging and photometry from the Spitzer Space Telescope, and published submillimetre CO J=3-2 maps of high-velocity molecular outflows. We detect and label 85 H2 features and associate these with 26 molecular outflows. Description: We use WFCAM data, Spitzer data and JCMT data. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea1.dat 96 85 H2 features in Perseus-West -------------------------------------------------------------------------------- See also: J/A+AS/106/165 : Near-IR imaging photometry of NGC 1333 (Aspin+ 1994) J/AJ/130/2212 : X-ray and NIR studies of L1448 (Tsujimoto+, 2005) J/ApJ/478/603 : L1448 + L1455 new Herbig-Haro flows (Bally+ 1997) Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- [DSL2008] H2 feature sequential number 4 I1 h RAh Rigth ascension (J2000.0) (1) 6- 7 I2 min RAm Rigth ascension (J2000.0) (1) 9- 14 F6.3 s RAs Rigth ascension (J2000.0) (1) 16 A1 --- DE- Declination sign (J2000.0) (1) 17- 18 I2 deg DEd Declination (J2000.0) (1) 20- 21 I2 arcmin DEm Declination (J2000.0) (1) 23- 27 F5.2 arcsec DEs Declination (J2000.0) (1) 29- 40 A12 --- Source ?=- Source candidate (2) 41- 44 I4 arcsec Length ? Distance from the source to the most distant knot (3) 46- 49 I4 deg PA [-180/180]? Position angle (4) 51- 54 A4 --- HH Associated HH object number (if any is known) 55 A1 --- u_HH [?] Uncertainty flag on HH 58- 76 A19 --- Com Comment 79- 90 A12 --- ONames Other identifiers (5) 93- 96 A4 --- Fig Figures in which the feature appears -------------------------------------------------------------------------------- Note (1): Position of the brightest knot within the H2 feature or flow. Note (2): Most likely source. Numbers refer to Table 3 in Jorgensen et al., (2007ApJ...656..293J 2007ApJ...656..293J), [JJK2007] NN in Simbad: * SVS 13 = [SVS76] NGC 1333 13 in Simbad * L1448-IRS1 = NAME LDN 1448 IRS 1 in Simbad A dash means there is no obvious source candidate. Note (3): If no known source, entire length of all knots. Note (4): Position angle, measured east of north, of an axis drawn from the source to the feature. Note (5): Previous names of H2 features. * ASR refers to sources from Aspin et al. (1994, Cat. J/A+AS/106/165) * HL refers to sources from Hodapp & Ladd (1995ApJ...453..715H 1995ApJ...453..715H) * MH refers to sources from Walawender et al. (2005AJ....130.1795W 2005AJ....130.1795W), [WBK2005] MH N in Simbad -------------------------------------------------------------------------------- Acknowledgements: Chris J. Davis, c.davis(at)jach.hawaii.edu
(End) Patricia Vannier [CDS] 23-Dec-2008
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