J/ApJ/619/L95      Star formation in Stephan's Quintet               (Xu+, 2005)

Ultraviolet emission and star formation in Stephan's Quintet. Xu C.K., Iglesias-Paramo J., Burgarella D., Rich R.M., Neff S.G., Lauger S., Barlow T.A., Bianchi L., Byun Y.-I., Forster K., Friedman P.G., Heckman T.M., Jelinsky P.N., Lee Y.-W., Madore B.F., Malina R.F., Martin D.C., Milliard B., Morrissey P., Schiminovich D., Siegmund O.H.W., Small T., Szalay A.S., Welsh B.Y., Wyder T.K. <Astrophys. J., 619, L95-L98 (2005)> =2005ApJ...619L..95X 2005ApJ...619L..95X
ADC_Keywords: Active gal. nuclei ; Interstellar medium ; Ultraviolet Keywords: galaxies: active - galaxies: interactions - galaxies: ISM - galaxies: starburst - intergalactic medium - stars: formation Abstract: We present the first Galaxy Evolution Explorer (GALEX) UV images of the well-known interacting group of galaxies, Stephan's Quintet (SQ). We detect widespread UV emission throughout the group. However, there is no consistent coincidence between UV structure and emission in the optical, Hα, or HI. Excluding the foreground galaxy NGC 7320 (Sd), most of the UV emission is found in regions associated with the two spiral members of the group, NGC 7319 and NGC 7318b, and the intragroup medium starburst SQ-A. The extinction-corrected UV data are analyzed to investigate the overall star formation activity in SQ. Description: SQ was observed by GALEX on 2003 August 23, 2003 September 5, and 2003 September 6 in five orbits, with total exposure time of 3327s. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 22 35 57.5 +33 57 36 Stephan's Quintet = HCG 92 ---------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 112 26 Star formation properties in HCG 92 regions -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 20 A20 --- Name Name of the region 21 A1 --- f_Name [*] contribution of AGN subtracted (1) 22- 26 A5 --- Reg Region number in FUV (see Fig.2a) 28- 32 F5.2 mag FUV FUV magnitude (1530Å), corrected for Galactic extinction (2) 34- 37 F4.2 mag e_FUV Error in FUV (2) 39- 43 F5.2 [Lsun] logL log(LFUV), FUV luminosity (2) (3) 45- 48 F4.2 [Lsun] e_logL Error in logL (2) 50- 55 F6.3 Msun/yr SFR ?=-9.9 Star formation rate from LFUV (2) (3) 57- 61 F5.3 Msun/yr e_SFR ?=0 Error in SFR (2) 63- 67 F5.2 mag F-N FUV-NUV color index (NUV: 2310Å), corrected for Galactic extinction (2) 69- 72 F4.2 mag e_F-N Error in F-N (2) 74- 77 F4.1 [yr] logtUV ?=-9.9 log(stellar age) derived from extinction corrected FUV-NUV color index (3) 79- 81 F3.1 [yr] e_logtUV ?=0 Error in logtUV 83- 87 F5.2 mag B-V ?=-9.9 B-V color index, corrected for Galactic extinction 89- 92 F4.2 mag e_B-V ?=0 Error in B-V 94- 97 F4.1 [yr] logtBV ?=-9.9 log(stellar age) derived from extinction corrected B-V color index (3) 99-101 F3.1 [yr] e_logtBV ?=0 Error in logtBV 103-107 F5.2 mag AFUV ?=-9.9 Internal extinction in the FUV band (3) 109-112 F4.2 mag e_AFUV ?=0 Error in AFUV -------------------------------------------------------------------------------- Note (1): The contribution from the AGN is subtracted from the UV, optical, and MIR flux densities. Note (2): Total values of the parameters: FUVtotal = 15.36±0.10mag logLtotal = 10.54±0.05LSun SFRtotal = 6.687±0.646MSun/yr F-Ntotal = 0.34±0.14mag Note (3): Corrected for both internal and Galactic extinction. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Marianne Brouty [CDS] 27-Jul-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