J/ApJ/628/789      IRAS03301+3057 water masers     (De Gregorio-Monsalvo+, 2005)

High-resolution molecular line observations of the environment of the class 0 source B1-IRS. De Gregorio-Monsalvo I., Chandler C.J., Gomez J.F., Kuiper T.B.H., Torrelles J.M., Anglada G. <Astrophys. J., 628, 789-799 (2005)> =2005ApJ...628..789D 2005ApJ...628..789D (SIMBAD/NED BibCode)
ADC_Keywords: Masers ; Interstellar medium Keywords: ISM: individual (B1-IRS) - ISM: jets and outflows - ISM: kinematics and dynamics - ISM: molecules - stars: formation - stars: pre-main-sequence Abstract: In this work we present VLA observations of the NH3, CCS, and H2O maser emission at 1cm from the star-forming region B1-IRS (IRAS 03301+3057) with ∼5" (=1750AU) of angular resolution. The CCS emission is distributed in three clumps around the central source. These clumps exhibit a velocity gradient from red- to blueshifted velocities toward B1-IRS, probably due to an interaction with the outflow from an embedded protostar. Description: Simultaneous observations of the JN=21-10 transition of CCS (with a rest frequency of 22344.033MHz) and the 616-523 transition of H2O (with a rest frequency of 22235.080MHz) were carried out on 2003 April 4 using the VLA in its D configuration. The phase center of these observations was 03:33:16.3+31:07:51 (J2000.0). In order to compare our water maser results with those at other epochs, we also retrieved earlier H2O data from the VLA archive. These observations were carried out on 1998 October 24 and 1999 February 26, in the CnB and CD configurations, respectively, for project AF354. These data have been published by Furuya et al. (2003ApJS..144...71F 2003ApJS..144...71F). The phase center of these observations was 03:33:16.030+31:07:34.05 (J2000.0). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 50 23 Water maser components on 2003 April 4 table2.dat 50 11 Water maser components on 1998 October 24 table3.dat 50 24 Water maser components on 1999 February 25 -------------------------------------------------------------------------------- See also: J/A+AS/120/283 : Water maser features in ultracompact HII regions (Hofner+ 1996) J/ApJ/581/325 : NGC 2071 water masers (Seth+, 2002) J/ApJ/615/702 : IC 133 water vapor maser (Argon+, 2004) Byte-by-byte Description of file: table1.dat table2.dat table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 h RAh Hour of Right Ascension (J2000.0) 4- 5 I2 min RAm Minute of Right Ascension (J2000.0) 7- 13 F7.4 s RAs Second of Right Ascension (J2000.0) 14 A1 --- DE- Sign of the Declination (J2000.0) 15- 16 I2 deg DEd Degree of Declination (J2000.0) 18- 19 I2 arcmin DEm Arcminute of Declination (J2000.0) 21- 26 F6.3 arcsec DEs Arcsecond of Declination (J2000.0) 28- 32 F5.3 arcsec e_pos ? Position uncertainty (2σ) (1) 33 A1 --- f_pos Flag on pos (2) 34- 39 F6.1 mJy S1cm Flux density at 1cm (1) 41- 45 F5.1 mJy e_S1cm Error in S1cm (2σ) 47- 50 F4.1 km/s VLSR Local standard of rest velocity of maser emission -------------------------------------------------------------------------------- Note (1): Relative position uncertainties with respect to the phase center ; the absolute position error of the phase center is ∼0.28" (Table 1). Relative position uncertainties with respect to the reference feature used for self-calibration (Tables 2 and 3). Note (2): Flag on pos, defined as follows: a = Reference feature. Absolute position error is ∼0.021". b = Reference feature. Absolute position error is ∼0.12". -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Marianne Brouty [CDS] 19-May-2006
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