J/A+A/547/A49       Herschel EPoS: high-mass overview        (Ragan+, 2012)

The Earliest Phases of Star Formation (EPoS) - A Herschel key program: The precursors to high-mass stars and clusters. Ragan S., Henning T., Krause O., Pitann J., Beuther H., Linz H., Tackenberg J., Balog Z., Hennemnan M., Launhardt R., Lippok N., Schmiedeke A., Schuller F., Steinacker J., Stutz A., Vasyunina T. <Astron. Astrophys. 547, A49 (2012)> =2012A&A...547A..49R 2012A&A...547A..49R
ADC_Keywords: Protostars ; Infrared sources ; Photometry, infrared ; YSOs Keywords: ISM: clouds - stars: formation, massive Abstract: Stars are born deeply embedded in molecular clouds. In the earliest embedded phases, protostars emit the bulk of their radiation in the far-infrared wavelength range, where Herschel is perfectly suited to probe at high angular resolution and dynamic range. In the high-mass regime, the birthplaces of protostars are thought to be in the high-density structures known as infrared-dark clouds (IRDCs). While massive IRDCs are believed to have the right conditions to give rise to massive stars and clusters, the evolutionary sequence of this process is not well-characterized. As part of the Earliest Phases of Star formation (EPoS) Herschel guaranteed time key program, we isolate the embedded structures within IRDCs and other cold, massive molecular clouds. We present the full sample of 45 high-mass regions which were mapped at PACS 70, 100, and 160um and SPIRE 250, 350, and 500um. In the present paper, we characterize a population of cores which appear in the PACS bands and place them into context with their host molecular cloud and investigate their evolutionary stage. Description: The core catalog giving the photometric parameters for 496 cores appearing as point sources in the Herschel PACS 70, 100, and 160 micron bands, with best-fit core mass, temperatures, and luminosities. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 67 45 IRDC (infrared-dark clouds) sample tablec.dat 108 496 Core catalog -------------------------------------------------------------------------------- See also: J/ApJ/639/227 : MSX IRDC candidate catalog (Simon+, 2006) J/ApJ/641/389 : Millimetric observations of IRDC cores (Rathborne+, 2006) J/ApJ/680/349 : Galactic distribution of IRDCs (Jackson+, 2008) J/ApJ/686/384 : 12CO, 13CO, C18O survey of IRDCs (Du+, 2008) J/MNRAS/399/1506 : IRDC cores in SCUBA Legacy Catalogue (Parsons+, 2009) J/ApJ/698/324 : Spitzer IRDCs (Ragan+, 2009) J/ApJ/715/310 : Early stages of star formation in IRDCs (Rathborne+, 2010) Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 16 A16 --- Name Full IRDC name 18- 25 F8.4 deg RAdeg Right ascension (J2000) of map center 27- 34 F8.4 deg DEdeg Declination (J2000) of map center 36- 40 F5.1 km/s Vlsr LSR Velocity 42- 45 F4.2 kpc Dist Kinematic distance 47- 50 F4.2 kpc E_Dist Positive uncertainty in distance 52- 55 F4.2 kpc e_Dist Negative uncertainty in distance 57- 61 I5 Msun Mcld ?=-9999 Mass of entire cloud (1) 63- 67 A5 --- r_Mcld Source of large scale map (2) -------------------------------------------------------------------------------- Note (1): Masses are computed with ATLASGAL 870µm, SCUBA 850µm or MAMBO 1.2mm data (see r_Mcld). In cases where no such maps were available, the entry is -9999. Note (2): Source of large scale map as follows: SCUBA = mass computed with SCUBA 850um data MAMBO = mass computed with MAMBO 1.2mm data ATGAL = mass computed with ATLASGAL 870um data -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablec.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 16 A16 --- Name IRDC name 18- 19 I2 --- Core Core ID number 21- 28 F8.4 deg RAdeg Right ascension (J2000) 30- 38 F9.5 deg DEdeg Declination (J2000) 40- 46 F7.3 Jy S24 ?=-99.999 Flux density at 24µm (1) 48- 54 F7.2 Jy S70 Flux density at 70µm 56- 62 F7.2 Jy S100 Flux density at 100µm 64- 71 F8.2 Jy S160 Flux density at 160µm 73- 74 I2 K Tcore Core temperature in Kelvin 76- 82 F7.1 Lsun Lcore Core luminosity in solar luminosities 84- 90 F7.2 Msun Mcore Core mass in solar masses 92-108 A17 --- catID Catalog ID (IRAS or MSX) (2) -------------------------------------------------------------------------------- Note (1): Data were not available at 24µm for all cores, and some positions were saturated in the Spitzer MIPS detector. In normal cases, the flux density in Janskys is given (0.0 for instances of no counterpart in available data). Otherwise: 999.999 = saturated source in Spitzer MIPS 24µm image -99.999 = no data available Note (2): Names of IRAS source or MSX source (Glll.lll+bb.bbbb) that best matches the core position, RAdeg, DEdeg. -------------------------------------------------------------------------------- Acknowledgements: Sarah Ragan, ragan(at)mpia.de
(End) Sarah Ragan [MPIA], Patricia Vannier [CDS] 30-Oct-2012
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