<=== observer ===> "RWATERS",\ "Waters, L.B.F.M.",\ "",\ "SRON Laboratory for Space Research Groningen",\ " ",\ "P.O. Box 800",\ "9700 AV ",\ "Groningen ",\ "The Netherlands",\ "31 50 634090",\ "31 50 634033",\ "rens@sron.rug.nl" <=== proposal ===> "POSTAGB", 1, 3,\ {"planetary nebulae",\ "stellar winds",\ "stellar evolution"},\ {"S.R. Pottasch",\ "Kapteyn Institute",\ "Groningen",\ "D.A. Beintema",\ "SRON Groningen",\ "H.J.G.L.M. Lamers",\ "SRON Utrecht",\ "N.R. Trams",\ "ESA-SSD",\ "ESTEC",\ "C. Waelkens",\ "Astronomical Institu",\ "University Leuven",\ "A.A. Zijlstra",\ "ESO",\ "Garching",\ "Germany",\ "T. de Jong",\ "SRON Groningen"} <=== title ===> Transition objects between Asymptotic Giant Branch and Planetary Nebula <=== abstract ===> SCIENTIFIC ABSTRACT The short-lived evolutionary phase of low and intermediate mass stars between the Asymptotic Giant Branch (AGB) and the Planetary Nebula (PN) stage is not well understood. The central star rapidly increases its effective temperature and decreases its radius at constant luminosity, while the mass loss rate, which was very high on the AGB, drops to much lower values. As the AGB remnant expands and cools, the central star becomes visible again and can be studied in detail. During the transition to the PN phase, the character of the stellar wind of the central star changes from a dust/pulsation driven one on the AGB, to a fast, radiation driven wind once the star reaches effective temperatures above about 20,000 K. The physics of this process is not well known, and may be related to the geometry of the outflow. It is by now well established that many transition objects show considerable deviations from spherical symmetry. These asymmetries may occur shortly before leaving the AGB, or result from the rapid evolution in this transition phase. It is unlikely that these asymmetries arise as a result of interacting winds, since the fast wind begins at much higher Teff. Another unknown is the post-AGB mass loss rate, which however is of considerable importance for the further evolution of the central star and nebula. If the mass loss rate exceeds the nuclear burning rate, then mass loss determines the speed of evolution towards the PN phase, much as mass loss dominates the AGB evolution. Estimates of post-AGB mass loss rates range between 1e(-9) to 1e(-6) M(sun)/yr, while nuclear burning rates range between 1e(-8) and 1e(-7) M(sun)/yr. If mass loss is important, it speeds up the post-AGB evolution and may allow the formation of low luminosity planetary nebulae. The infrared HI recombination lines allow us to determine the amount of ionized circumstellar gas and from that the post-AGB mass loss rates. Study of the AGB remnant yields information on the mass loss history of the star while it was on the AGB. When the energy distribution is accuraty known, it can be modeled in detail and a kinematic age of the AGB remnant can be determined. This age can be compared to the evolutionary timescale of the central star, i.e. the time it took the star to reach its present Teff. These data are critical tests of current evolutionary tracks for post-AGB stars, especially when combined with optical and UV abundance studies of the stellar photosphere. Post-AGB stars also allow us to study the changes in the dust properties as the temperature of the central star changes from very low to very high values. In several post-AGB stars the unidentified 21 mu feature is seen, as well as the PAH features at 3.3, 7.7, 8.6, and 11.3 mu. It is clear that post-AGB stars can be studied best in the (far)-IR. ISO is the only instrument that allows a study of the IR properties of the ionized and molecular outflow of the star, and of the properties of the circumstellar dust. OBSERVATION SUMMARY. We propose to obtain SWS full scans at reduced resolution of a sample of post-AGB stars with a range in chemical composition, luminosity, temperature and geometry. Sample selection is mainly based on IRAS data and follow-up observations. In addition, we propose to obtain PHT-S spectra of all our targets. For several stars we request full resolution SWS scans (SWS AOT01). <=== scientific_justification ===> Time distribution for spring launch targets Team: top 40% second 30% last 30% SWS 13930 12840 6144 Time distribution for autumn launch targets Team: top 40% second 30% last 30% SWS 14278 7896 14796 Table 1. Cross-references source names -------------------------------------------------------------------------- name 1 name 2 name 3 1 CRL 618 2 HD 44179 Red Rectangle 3 HD 56126 4 U Mon HD 5 IRAS08005-2356 6 IRAS09371+1212 Frosty Leo 7 HR 4049 HD 89353 8 HD 101584 9 R CrB HD 141527 10 HD 161796 11 89 Her HD 85545 12 AC Her HD 13 IRC +10420 14 CRL 2688 15 SAO 34504 HD235858 C-rich 21 mic, group V K star 16 OH231.8+4.2 17 HD 213985 18 IRAS17347-3139 19 IRAS17579-3121 20 IRAS17418-2713 21 AFGL 4106 22 IRAS04296+3429 21mic, C-rich, V 23 IRAS09425-6040 IIIb, young ppn 24 C*1662 C star in region V! 25 Roberts 22 pah, V, A2Iab 26 CD-49 11554 Be 27 IRAS17583-2201 IIIb, young ppn 28 OH17.7-2.0 O-rich, V 29 AFGL 5502 VIII, C-rich 30 HD 179821 O-rich, V, G5 31 HD 187885 C-rich, V, F2/3Iab+A 32 IRAS20028+3910 33 IRAS22223+4327 C-rich, V 34 IRAS23304+6147 C-rich, 21mic., group V -------------------------------------------------------------------------- Table 2. Positions and Offsets -------------------------------------------------------------------------- No ra dec precision offset ref. pos window 1950.0 (",") (") 1 04 39 32.9 +36 01 09 1,1 0 spr 2 06 17 36.9 -10 36 51 1,1 0 1 spr 3 07 13 25.4 +10 05 08 1,1 0 1 spr 4 07 28 24.2 -09 40 14 1,1 0 1 spr 5 08 00 00 -23 56 00 5,15 0 2 spr 6 09 37 12.0 +12 12 31 5,15 0 2 spr 7 10 15 49.9 -28 44 29 1,1 0 1 saf 8 11 38 33.7 -55 17 48 1,1 0 1 saf 9 15 46 30.6 +28 18 31 1,1 0 1 aut 10 17 43 41.3 +50 03 47 1,1 0 1 aut 11 17 53 24.1 +26 03 23 1,1 0 1 aut 12 18 28 08.9 +21 49 52 1,1 0 1 aut 13 19 24 26.7 +11 15 11 1,1 0 saf 14 21 00 16.0 +36 30 00 5,15 0 saf 15 22 27 13.4 +54 35 44 1,1 0 1 saf 16 07 39 58.9 -14 35 44 1,1 0 spr 17 22 32 46.0 -17 30 59 1,1 0 1 saf 18 17 34 45.9 -31 39 11 5,15 0 2 aut 19 17 57 59.7 -31 22 01 5,15 0 2 aut 20 17 41 51.9 -27 13 33 5,15 0 2 aut 21 10 21 32.5 -59 16 53 3,3 0 4 saf 22 04 29 40.3 +34 29 53 3,3 0 4 spr 23 09 42 35.2 -60 40 34 3,3 0 4 saf 24 10 17 48.6 -59 58 23 3,3 0 4 saf 25 10 19 45.1 -57 50 28 3,3 0 4 saf 26 17 31 11.2 -49 24 25 3,3 0 4 aut 27 17 58 21.6 -22 01 05 3,3 0 4 aut 28 18 27 39.8 -14 31 04 3,3 0 4 aut 29 18 30 50.8 -05 03 27 3,3 0 4 aut 30 19 11 24.9 +00 02 19 3,3 0 4 aut 31 19 50 00.7 -17 09 38 3,3 0 4 saf 32 20 02 48.0 +39 10 03 3,3 0 4 aut 33 22 22 22.9 +43 27 49 3,3 0 4 saf 34 23 30 26.7 +61 47 15 3,3 0 4 saf -------------------------------------------------------------------------- References for positions and accuracy 1: SAO Catalogue 2: IRAS Point Source Catalogue 3: Kwok et al. 1987 4: Loup, Thesis, Grenoble 1991 Table 4. Photometric data (fluxes in Jansky) -------------------------------------------------------------------------- no ident J H K L M 12 25 60 -------------------------------------------------------------------------- 1 CRL 618 0.02 0.13 2.53 13.64 470 1106 1035 2 HD 44179 4.11 10.90 26.47 86.79 113.46 422 456 173 3 HD 56126 2.79 2.19 1.66 0.73 - 25 117 50 4 U Mon 29.75 29.20 23.06 23.04 34.26 124 88.4 26.6 5 IRAS08005-2356 1.04 2.08 4.20 12.09 13.27 17.96 51.8 29.83 6 IRAS09371+1212 - - - - - <0.3 4.6 70.3 7 HR 4049 22.16 25.20 39.34 79.16 75.66 31.5 6.81 1.35 8 HD 101584 7.20 9.94 20.27 40.41 46.43 88.7 133.7 177.4 9 R CrB 15.76 12.87 13.52 63.46 65.29 38.9 17.1 3.94 10 HD 161796 7.61 4.42 2.60 1.29 - 6.65 188.9 128.8 11 89 Her 25.91 23.85 32.42 60.05 70.93 97.6 54.1 13.2 12 AC Her 6.69 6.75 5.14 3.65 5.95 41.4 65.3 21.4 13 IRC+10 420 16.35 36.09 41.96 157 285 1346 2314 718 14 CRL 2688 0.26 0.21 0.50 1.01 5.95 b r i g h t 15 SAO 34504 12.29 11.21 8.61 5.23 4.69 73.9 302 96.6 16 OH231.8+4.2 0.48 1.30 2.22 4.55 - 19.0 226 548 17 HD 213985 0.85 0.93 1.32 2.45 2.34 4.90 4.04 1.82 18 IRAS17347-3139 - - 0.03 0.64 0.78 18.99 100.30 125.40 19 IRAS17579-3121 - - - - - 2.01 62.39 58.21 20 IRAS17418-2713 - - - - - 14.95 51.28 45.94 21 AFGL 4106 23.4 43.8 41.1 25.7 - 22 IRAS04296+3429 0.23 0.38 0.35 0.33 0.50 12.7 45.9 15.4 23 IRAS09425-6040 - - - - - 26.8 55.5 21.2 24 C*1662 - - - - - 4.12 38.3 76.1 25 Roberts 22 - - - - - 200 1090 588 26 CD-49 11554 0.22 0.19 0.16 0.16 0.31 18.3 151 58.7 27 IRAS17583-2201 - - - - - 51.5 79.7 29.9 28 OH17.7-2.0 0.04 0.068 0.12 0.44 0.78 22.6 132 120 29 AFGL 5502 - - - - - 28.3 162 677 30 HD 179821 16.4 17.0 12.9 6.64 5.38 31.3 648 516 31 HD 187885 2.2 1.86 1.27 0.65 0.57 27.8 165 73.4 32 IRAS20028+3910 - - - - - 41.8 211 143 33 IRAS22223+4327 - m=9.1 m=8.4 m=5.1 - 2.12 37.1 22.4 34 IRAS23304+6147 0.62 0.80 0.57 0.40 0.48 11.4 59.1 26.6 -------------------------------------------------------------------------- Table 5. Priorities, Time and Coordination with other consortia. -------------------------------------------------------------------------- Other observations no ident prio AOT time LWS CAM PHT needed in SWS time: -------------------------------------------------------------------------- 1 CRL 618 1 SWS01 1116 + + + 2 HD 44179 1 SWS01 3600 + + + 3 HD 56126 2 SWS01 1116 + PHT-S PHT40 120 4 U Mon 2 SWS01 1116 + + PHT-S PHT40 120 5 IRAS08005-2356 2 SWS01 1116 PHT-S PHT40 120 6 IRAS09371+1212 2 SWS01 1116 + + PHT-S 7 HR 4049 1 SWS01 1116 + 8 HD 101584 2 SWS01 1116 + PHT40 120 9 R CrB 2 SWS01 1116 + + + PHT-S 10 HD 161796 1 SWS01 1116 + + PHT-S PHT40 120 11 89 Her 1 SWS01 1116 + PHT-S PHT40 120 12 AC Her 1 SWS01 1116 + + PHT-S PHT40 120 13 IRC+10420 1 SWS01 1906 + + PHT40 120 14 CRL 2688 1 SWS01 3600 + + + PHT40 120 15 SAO 34504 2 SWS01 1116 + + PHT-S PHT40 120 16 OH231.8+4.2 1 SWS01 1116 + + + PHT-S 17 HD 213985 3 SWS01 1116 + + PHT-S PHT40 120 18 IRAS17347-3139 3 SWS01 1116 + PHT-S PHT40 120 19 IRAS17579-3121 3 SWS01 1116 PHT-S PHT40 120 20 IRAS17418-2713 3 SWS01 1116 PHT-S PHT40 120 21 AFGL 4106 2 SWS01 1116 PHT-S,LWS PHT40 120 LWS01 600 22 IRAS04296+3429 2 SWS01 1116 + PHT-S PHT40 120 23 IRAS09425-6040 3 SWS01 1116 PHT-S PHT40 120 24 C* 1662 3 SWS01 1116 PHT-S,LWS PHT40 120 LWS01 600 25 Roberts 22 3 SWS01 1116 PHT-S,LWS PHT40 120 LWS01 600 26 CD-49 11554 3 SWS01 1116 PHT-S PHT40 120 27 IRAS17583-2201 3 SWS01 1116 PHT-S PHT40 120 28 OH17.7-2.0 1 SWS01 1116 + PHT-S PHT40 120 29 AFGL 5502 3 SWS01 1116 PHT-S PHT40 120 30 HD 179821 1 SWS01 1116 + PHT-S PHT40 120 31 HD 187885 2 SWS01 1116 + PHT-S PHT40 120 32 IRAS20028+3910 3 SWS01 1116 + PHT-S PHT40 120 33 IRAS22223+4327 2 SWS01 1116 PHT-S PHT40 120 34 IRAS23304+6147 1 SWS01 1116 + PHT-S PHT40 120 -------------------------------------------------------------------------- <=== autumn_launch_targets ===> 1, "SWS01",1.,"N","HR 4049 ", 10.26386, -28.74139, 1950, 0.,0., 1116, 0 2, "SWS01",2.,"N","HD 101584 ", 11.64269, -55.29667, 1950, 0.,0., 1116, 3 3, "PHT40",2.,"N","HD 101584 ", 11.64269, -55.29667, 1950, 0.,0., 120, 0 4, "SWS01",2.,"N","R CrB ", 15.77517, 28.30861, 1950, 0.,0., 1116, 0 5, "SWS01",1.,"N","HD 161796 ", 17.72814, 50.06306, 1950, 0.,0., 1116, 6 6, "PHT40",1.,"N","HD 161796 ", 17.72814, 50.06306, 1950, 0.,0., 120, 0 7, "SWS01",1.,"N","89 Her ", 17.89003, 26.05639, 1950, 0.,0., 1116, 8 8, "PHT40",1.,"N","89 Her ", 17.89003, 26.05639, 1950, 0.,0., 120, 0 9, "SWS01",1.,"N","AC Her ", 18.46914, 21.83111, 1950, 0.,0., 1116, 10 10, "PHT40",1.,"N","AC Her ", 18.46914, 21.83111, 1950, 0.,0., 120, 0 11, "SWS01",1.,"N","IRC+10420 ", 19.40742, 11.25306, 1950, 0.,0., 1906, 12 12, "PHT40",1.,"N","IRC+10420 ", 19.40742, 11.25306, 1950, 0.,0., 120, 0 13, "SWS01",1.,"N","CRL 2688 ", 21.00444, 36.50000, 1950, 0.,0., 3600, 14 14, "PHT40",1.,"N","CRL 2688 ", 21.00444, 36.50000, 1950, 0.,0., 120, 0 15, "SWS01",2.,"N","SAO 34504 ", 22.45372, 54.59556, 1950, 0.,0., 1116, 16 16, "PHT40",2.,"N","SAO 34504 ", 22.45372, 54.59556, 1950, 0.,0., 120, 0 17, "SWS01",3.,"N","HD 213985 ", 22.54611, -17.51639, 1950, 0.,0., 1116, 18 18, "PHT40",3.,"N","HD 213985 ", 22.54611, -17.51639, 1950, 0.,0., 120, 0 19, "SWS01",3.,"N","IRAS17347-3139", 17.57942, -31.65306, 1950, 0.,0., 1116, 20 20, "PHT40",3.,"N","IRAS17347-3139", 17.57942, -31.65306, 1950, 0.,0., 120, 0 21, "SWS01",3.,"N","IRAS17579-3121", 17.96658, -31.36694, 1950, 0.,0., 1116, 22 22, "PHT40",3.,"N","IRAS17579-3121", 17.96658, -31.36694, 1950, 0.,0., 120, 0 23, "SWS01",3.,"N","IRAS17418-2713", 17.69775, -27.22583, 1950, 0.,0., 1116, 24 24, "PHT40",3.,"N","IRAS17418-2713", 17.69775, -27.22583, 1950, 0.,0., 120, 0 25, "SWS01",2.,"N","AFGL 4106 ", 10.35903, -59.28139, 1950, 0.,0., 1116, 26 26, "PHT40",2.,"N","AFGL 4106 ", 10.35903, -59.28139, 1950, 0.,0., 120, 27 27, "LWS01",2.,"N","AFGL 4106 ", 10.35903, -59.28139, 1950, 0.,0., 600, 0 28, "SWS01",3.,"N","IRAS09425-6040", 9.70978, -60.67611, 1950, 0.,0., 1116, 29 29, "PHT40",3.,"N","IRAS09425-6040", 9.70978, -60.67611, 1950, 0.,0., 120, 0 30, "SWS01",3.,"N","C* 1662 ", 10.29683, -59.97306, 1950, 0.,0., 1116, 31 31, "PHT40",3.,"N","C* 1662 ", 10.29683, -59.97306, 1950, 0.,0., 120, 32 32, "LWS01",3.,"N","C* 1662 ", 10.29683, -59.97306, 1950, 0.,0., 600, 0 33, "SWS01",3.,"N","Roberts 22 ", 10.32919, -57.84111, 1950, 0.,0., 1116, 34 34, "PHT40",3.,"N","Roberts 22 ", 10.32919, -57.84111, 1950, 0.,0., 120, 35 35, "LWS01",3.,"N","Roberts 22 ", 10.32919, -57.84111, 1950, 0.,0., 600, 0 36, "SWS01",3.,"N","CD-49 11554 ", 17.51978, -49.40694, 1950, 0.,0., 1116, 37 37, "PHT40",3.,"N","CD-49 11554 ", 17.51978, -49.40694, 1950, 0.,0., 120, 0 38, "SWS01",3.,"N","IRAS17583-2201", 17.97267, -22.01806, 1950, 0.,0., 1116, 39 39, "PHT40",3.,"N","IRAS17583-2201", 17.97267, -22.01806, 1950, 0.,0., 120, 0 40, "SWS01",1.,"N","OH17.7-2.0 ", 18.46106, -14.51778, 1950, 0.,0., 1116, 41 41, "PHT40",1.,"N","OH17.7-2.0 ", 18.46106, -14.51778, 1950, 0.,0., 120, 0 42, "SWS01",3.,"N","AFGL 5502 ", 18.51411, -5.05750, 1950, 0.,0., 1116, 43 43, "PHT40",3.,"N","AFGL 5502 ", 18.51411, -5.05750, 1950, 0.,0., 120, 0 44, "SWS01",1.,"N","HD 179821 ", 19.19025, 0.03861, 1950, 0.,0., 1116, 45 45, "PHT40",1.,"N","HD 179821 ", 19.19025, 0.03861, 1950, 0.,0., 120, 0 46, "SWS01",2.,"N","HD 187885 ", 19.83353, -17.16056, 1950, 0.,0., 1116, 47 47, "PHT40",2.,"N","HD 187885 ", 19.83353, -17.16056, 1950, 0.,0., 120, 0 48, "SWS01",3.,"N","IRAS20028+3910", 20.04667, 39.16750, 1950, 0.,0., 1116, 49 49, "PHT40",3.,"N","IRAS20028+3910", 20.04667, 39.16750, 1950, 0.,0., 120, 0 50, "SWS01",2.,"N","IRAS22223+4327", 22.37303, 43.46361, 1950, 0.,0., 1116, 51 51, "PHT40",2.,"N","IRAS22223+4327", 22.37303, 43.46361, 1950, 0.,0., 120, 0 52, "SWS01",1.,"N","IRAS23304+6147", 23.50742, 61.78750, 1950, 0.,0., 1116, 53 53, "PHT40",1.,"N","IRAS23304+6147", 23.50742, 61.78750, 1950, 0.,0., 120, 0 <=== spring_launch_targets ===> 1, "SWS01",1.,"N","CRL 618 ", 4.65914, 36.01917, 1950, 0.,0., 1116, 0 2, "SWS01",1.,"N","HD 44179 ", 6.29358, -10.61417, 1950, 0.,0., 3600, 0 3, "SWS01",2.,"N","HD 56126 ", 7.22372, 10.08556, 1950, 0.,0., 1116, 4 4, "PHT40",2.,"N","HD 56126 ", 7.22372, 10.08556, 1950, 0.,0., 120, 0 5, "SWS01",2.,"N","U Mon ", 7.47339, -9.67056, 1950, 0.,0., 1116, 6 6, "PHT40",2.,"N","U Mon ", 7.47339, -9.67056, 1950, 0.,0., 120, 0 7, "SWS01",2.,"N","IRAS08005-2356", 8.00000, -23.93333, 1950, 0.,0., 1116, 8 8, "PHT40",2.,"N","IRAS08005-2356", 8.00000, -23.93333, 1950, 0.,0., 120, 0 9, "SWS01",2.,"N","IRAS09371+1212", 9.62000, 12.20861, 1950, 0.,0., 1116, 0 10, "SWS01",1.,"N","HR 4049 ", 10.26386, -28.74139, 1950, 0.,0., 1116, 0 11, "SWS01",2.,"N","HD 101584 ", 11.64269, -55.29667, 1950, 0.,0., 1116, 12 12, "PHT40",2.,"N","HD 101584 ", 11.64269, -55.29667, 1950, 0.,0., 120, 0 13, "SWS01",1.,"N","IRC+10420 ", 19.40742, 11.25306, 1950, 0.,0., 1906, 14 14, "PHT40",1.,"N","IRC+10420 ", 19.40742, 11.25306, 1950, 0.,0., 120, 0 15, "SWS01",1.,"N","CRL 2688 ", 21.00444, 36.50000, 1950, 0.,0., 3600, 16 16, "PHT40",1.,"N","CRL 2688 ", 21.00444, 36.50000, 1950, 0.,0., 120, 0 17, "SWS01",2.,"N","SAO 34504 ", 22.45372, 54.59556, 1950, 0.,0., 1116, 18 18, "PHT40",2.,"N","SAO 34504 ", 22.45372, 54.59556, 1950, 0.,0., 120, 0 19, "SWS01",1.,"N","OH231.8+4.2 ", 7.66636, -14.59556, 1950, 0.,0., 1116, 0 20, "SWS01",3.,"N","HD 213985 ", 22.54611, -17.51639, 1950, 0.,0., 1116, 21 21, "PHT40",3.,"N","HD 213985 ", 22.54611, -17.51639, 1950, 0.,0., 120, 0 22, "SWS01",2.,"N","AFGL 4106 ", 10.35903, -59.28139, 1950, 0.,0., 1116, 23 23, "PHT40",2.,"N","AFGL 4106 ", 10.35903, -59.28139, 1950, 0.,0., 120, 24 24, "LWS01",2.,"N","AFGL 4106 ", 10.35903, -59.28139, 1950, 0.,0., 600, 0 25, "SWS01",2.,"N","IRAS04296+3429", 4.49453, 34.49806, 1950, 0.,0., 1116, 26 26, "PHT40",2.,"N","IRAS04296+3429", 4.49453, 34.49806, 1950, 0.,0., 120, 0 27, "SWS01",3.,"N","IRAS09425-6040", 9.70978, -60.67611, 1950, 0.,0., 1116, 28 28, "PHT40",3.,"N","IRAS09425-6040", 9.70978, -60.67611, 1950, 0.,0., 120, 0 29, "SWS01",3.,"N","C* 1662 ", 10.29683, -59.97306, 1950, 0.,0., 1116, 30 30, "PHT40",3.,"N","C* 1662 ", 10.29683, -59.97306, 1950, 0.,0., 120, 31 31, "LWS01",3.,"N","C* 1662 ", 10.29683, -59.97306, 1950, 0.,0., 600, 0 32, "SWS01",3.,"N","Roberts 22 ", 10.32919, -57.84111, 1950, 0.,0., 1116, 33 33, "PHT40",3.,"N","Roberts 22 ", 10.32919, -57.84111, 1950, 0.,0., 120, 34 34, "LWS01",3.,"N","Roberts 22 ", 10.32919, -57.84111, 1950, 0.,0., 600, 0 35, "SWS01",2.,"N","HD 187885 ", 19.83353, -17.16056, 1950, 0.,0., 1116, 36 36, "PHT40",2.,"N","HD 187885 ", 19.83353, -17.16056, 1950, 0.,0., 120, 0 37, "SWS01",2.,"N","IRAS22223+4327", 22.37303, 43.46361, 1950, 0.,0., 1116, 38 38, "PHT40",2.,"N","IRAS22223+4327", 22.37303, 43.46361, 1950, 0.,0., 120, 0 39, "SWS01",1.,"N","IRAS23304+6147", 23.50742, 61.78750, 1950, 0.,0., 1116, 40 40, "PHT40",1.,"N","IRAS23304+6147", 23.50742, 61.78750, 1950, 0.,0., 120, 0