J/ApJ/755/20     YSOs population of Sh2-294 with Spitzer/IRAC     (Samal+, 2012)

Star formation and young population of the H II complex Sh2-294. Samal M.R., Pandey A.K., Ojha D.K., Chauhan N., Jose J., Pandey B. <Astrophys. J., 755, 20 (2012)> =2012ApJ...755...20S 2012ApJ...755...20S
ADC_Keywords: Photometry, infrared ; H II regions ; YSOs ; Stars, masses ; Stars, ages Keywords: H II regions; ISM: individual: Sh2-294; stars: formation; stars: pre-main sequence Abstract: The Sh2-294 H II region ionized by a single B0V star features several infrared excess sources, a photodissociation region, and also a group of reddened stars at its border. The star formation scenario in this region seems to be quite complex. In this paper, we present follow-up results of Sh2-294 H II region at 3.6, 4.5, 5.8, and 8.0µm observed with the Spitzer Space Telescope Infrared Array Camera (IRAC), coupled with H2(2.12µm) observation, to characterize the young population of the region and to understand its star formation history. We identified 36 young stellar object (YSO, Class I, Class II, and Class I/II) candidates using IRAC color-color diagrams. It is found that Class I sources are preferentially located at the outskirts of the H II region and associated with enhanced H2emission; none of them are located near the central cluster. Combining the optical to mid-infrared (MIR) photometry of the YSO candidates and using the spectral energy distribution fitting models, we constrained stellar parameters and the evolutionary status of 33 YSO candidates. Most of them are interpreted by the model as low-mass (<4 M) YSOs; however, we also detected a massive YSO (∼9 M) of Class I nature, embedded in a cloud of visual extinction of ∼24 mag. Description: The archived MIR data for the region were obtained with the Infrared Array Camera (IRAC) on board the Spitzer Space Telescope. The IRAC observations of the region were taken on 2006 November 25 (Program ID 30734, AOR key 18902784: Massive Star Clusters, PI: Donald Figer). Restricting our analysis to the sources having photometric error less than 0.2 mag, we detected 102 sources in the 3.6, 4.5, and 5.8um bands and 31 sources in all the IRAC bands in a common area of ∼6.8'x6.8'. These catalogs are made after removing three sources that appear to be extended and/or multiple sources in the high-resolution H2 (2.12um) and 3.6um IRAC images. The final catalog used to identify the YSOs in the present analysis is given in Table 1. The H2 mosaic image was constructed using the observations made with the ISAAC camera of the Very Large Telescope (VLT). The data were retrieved from the ESO archive. Further details about the observations are described in Yun et al. (2008, Cat. J/A+A/483/209). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 72 103 Photometric data in IRAC bands (97 different positions) table2.dat 97 33 Inferred physical parameters from SED fits to YSOs -------------------------------------------------------------------------------- See also: V/114 : MSX6C Infrared Point Source Catalog (Egan+ 2003) II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) VII/50 : CO Radial Velocities Toward Galactic H II Regions (Blitz+ 1982) J/A+A/483/209 : Phot. of a stellar cluster near IRAS 07141-092 (Yun+, 2008) J/A+A/470/161 : UBV photometry of HII regions exciting stars (Russeil+, 2007) J/ApJ/649/759 : Bubbles in the galactic disk (Churchwell+, 2006) J/A+A/397/213 : Galactic HII regions (Paladini+, 2003) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 F9.5 deg RAdeg [109.0/109.2] Right Ascension (J2000) 10 A1 --- --- [0] 12- 19 F8.5 deg DEdeg [-9.5/-9.3] Declination (J2000) 20 A1 --- --- [0] 22- 27 F6.3 mag 3.6mag [9.6/15] Spitzer/IRAC 3.6 micron band magnitude 29- 33 F5.3 mag e_3.6mag Uncertainty in 3.6mag 35- 40 F6.3 mag 4.5mag [9.2/14.8] Spitzer/IRAC 4.5um band magnitude 42- 46 F5.3 mag e_4.5mag Uncertainty in 4.5mag 48- 53 F6.3 mag 5.8mag [7.8/14.1] Spitzer/IRAC 5.8um band magnitude 55- 59 F5.3 mag e_5.8mag Uncertainty in 5.8mag 61- 66 F6.3 mag 8.0mag [8.6/12.4]? Spitzer/IRAC 8.0um band magnitude 68- 72 F5.3 mag e_8.0mag [0.02/0.2]? Uncertainty in 8.0mag -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 A2 --- ID YSO identification (1) 4- 13 F10.6 deg RAdeg [109/109.2] Right ascension (J2000) 15- 23 F9.6 deg DEdeg [-9.5/-9.3] Declination (J2000) 25- 28 F4.2 Msun M [0.6/8.8] Stellar mass 30- 33 F4.2 Msun e_M [0.1/2] Mass uncertainty 35- 39 F5.2 kK T [3.4/16.1] Stellar temperature 41- 44 F4.2 kK e_T [0.1/5] Temperature uncertainty 46- 49 F4.2 Myr Age [0.04/8.1] Stellar age (t*) 51- 54 F4.2 Myr e_Age [0.04/3.3] Age uncertainty 56- 60 F5.3 Msun Mdisk [0/0.2] Disk mass 62- 66 F5.3 Msun e_Mdisk [0/0.3] Mdisk uncertainty 68- 73 F6.2 10-8Msun/yr dM/dt [0/390] Disk accretion rate (dM/dtdisk) 75- 80 F6.2 10-8Msun/yr e_dM/dt [0/383] dM/dt uncertainty 82- 86 F5.2 mag Av [3.1/23.7] Foreground visual absorption 88- 91 F4.2 mag e_Av [0.1/6.7] Av uncertainty 93- 97 F5.2 --- chi2 [0.8/35.9] Best fit χ2min -------------------------------------------------------------------------------- Note (1): The IRAC-classified Class II, Class I/II, and Class I YSOs are labeled with the numbers 1-25, T1-T5, and C1-C3, respectively (see Figure 3). -------------------------------------------------------------------------------- History: From electronic version of the journal References: Samal et al. Paper I. 2007ApJ...671..555S 2007ApJ...671..555S
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 06-Mar-2014
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