J/A+AS/93/121ivo://CDS.VizieR/J/A+AS/93/121CDSNyman L.A.Booth R.S.Carlstroem U.Habing H.J.Heske A.Sahai R.,Stark R.van der Veen W.E.C.J.Winnberg A.2018-01-04T08:22:03Z2008-04-11T09:03:29ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frinfrared-sourceslate-type-starsstellar-mass-lossThe first results from a survey of circumstellar CO(1-0) emission are presented. The sources were selected from the IRAS point source catalog according to the IRAS color criteria described in van der Veen and Habing (1988A&A...194..125V). The sources have good quality fluxes at 12, 25, and 60 microns, flux densities larger than 20Jy at 25{mu}m, and are situated more than 5{deg} away from the Galactic plane. The survey is undertaken to study the relationship between mass loss rates, dust properties, and the evolution along the AGB. The sample consists of 787 sources and contains both oxygen and carbon-rich stars, including Mira variables, OH/IR objects, protoplanetary nebulae, planetary nebulae, and 60-micron excess sources. So far, 519 objects, situated on both the northern and the southern sky, have been observed; 163 sources were found to have circumstellar CO emission, and in 58 of these CO emission has not previously been detected.1992A&AS...93..121Nhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/93/121CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/93/121https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/93/121http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/93/121https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/93/121https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/93/121http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/93/121GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+AS/93/121/table4 (Detected and undetected sources)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+AS/93/121/table4?https://vizier.iucaa.in/viz-bin/conesearch/J/A+AS/93/121/table4?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+AS/93/121/table4?GETtext/xml+votable180.050000true1.72077843.0832240.0055555555555555566/220 354 646 676 765 883 889 957-958 1003 1078-1079 1168-1169 1182 1217 1229 1231 1238 1371 1399 1490 1493 1501 1507-1508 1619 1634 1647 1727 1731 1734 1889 1892 1974 1977 1986 2031 2084 2203 2428 2500 2528 2694 2732 2795 2961 2982 2990 3243 3352 3359 3438 3446 3459 3469 3491 3765-3766 3801 3819 3829 3849 3856 3951 4018 4290 4306 4347 4365 4614 4635 4690 4892 4972 5273 5489 5647 6007 6251 6383 6444 6714 6803 6813 6884 6890 6919 7119 7152 7619 7631 7673 7758 7827 7919 8297 8475 8492 8532 8603 8926 9074 9137 9142 9233 9258 9423 9713 9750 9783 9813 9939 9968 10074 10103 10137 10167 10628 10635 10960 11165 11597 11605 11747 11866 11928 12137 12334 12363 12556 12833 12882 12999 13210 13297 13463 13615 13666 13676-13677 13683 13711 13783 13813 13845 13861 13875 13917 13968 14005 14159 14161 14175 14371 14399 14443 14473 14508 14550 14567 14738 14765 14811 14834 14846 14988 15044 15105 15122 15170 15172 15492 15554 15657 15663 15718 15737 15741 15752 15757 16019 16088 16132 16147 16157 16175 16224 16232-16233 16318 16459 16783 17192 17271 17716 18364 18457 18634 18998 19112 19279 19293 19490 20022 20212 20272 20626 20699 20715 20843 20965 21050 21215 21224 21241 21255 21316 21326 21338 21396 21456 21458 21464 21494 21777 21854 21878 21931 21977 22051 22144 22333 22392 22425 22556 22806 22860 22941 23013 23095 23327 23470 23549 23606 23611 23831 24098 24258 24389 24443 24563 25228 25246 25798 25864 26070 26180 26289 26319 26327 26345 26654 28154 28188 28675 28685 28727 28772 28971 28994 29000 29023 29072 29129 29136 29146 29189 29196 29213 29286 29308 29310 29331 29438 29545 29589 29597 29626 29660 29662 29701 29705 29817 29855 29877 29886 29963 30011 30034 30069 30087 30123 30303 30397 30440 30445 30472 30494 30787 30795 30802-30803 31086 31194 31231 31292 31366 31464 31775 31828 31837 31849 31866 31938 32009 32062 32110 32114 32142 32181 32189 32254 32259 32271 32331 32527 32543 32562 32614 32626 32723 32771 32784 32790 32799 33056 33097 33140 33589 33624 33739 33919 34279 34312 34576 34792 35506 36028 36222 36320 36322 36369 36954 36956 36986 37006 37139 37186 37220 37306-37307 37352 37354 37400 37405 37617 37659 37675 37970 38130 38149 38197 38230 38505-38506 38660 38701 39323 39342 39355 39448 39504 39631 39637 39724 39738 39860 39905 40235 40422 40502 40566 40601 40686 40847 40858 41045 41118 41174 41198 41204 41245 41310 41328 41358 41371 41394 41434 41472 41530 41542 41571 41904 41937 41945 41953 41962 41967 41974 41996 42044 42057 42094 42109 42124 42196 42254 42281 42285 42332 42337 42479 42527 42556 42584 42597 42621 42632 42730 42757 42761 42773 42840-42841 42872 42895 42919 43085-43086 43092 43132 43174 43198 43235 43494 43572 43581 43726 44018 44198 44417 44857 45075 45279 45285 45291 45343 45782 45809 45824 46138 46160 46313 46318 46330 46387 46795 46932 46938 47248 47303 47332 47342 47414 47508 47637 47664 47737 47826 47963 48006 48038 48073 48097 48133 48301 48604 48650 48700 48822 48860 48903 489512.4696718532768785e-21 2.1346512726771855e-20https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+AS/93/121?format=asciiInfraredRadiodefaultJ/A+AS/93/121/table4Detected and undetected sourcesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintT[abc] Table indicator: a=detected, b=tentative, c=not detected.meta.id;meta.datasetcharIRASIRAS Source Namemeta.id;meta.maincharprimaryn_IRASSimbad column added by the CDSmeta.ref.urlcharRegionin the IRAS two color diagram as defined by van der Veen & Habing, 1988A&A...194..125Vobs.fieldcharF12IRAS 12 micrometer flux densityJyphot.flux.density;em.IR.8-15umfloatF25IRAS 25 micrometer flux densityJyphot.flux.density;em.IR.15-30umfloatF60IRAS 60 micrometer flux densityJyphot.flux.density;em.IR.30-60umfloatrms? Rms noise the CO spectrum, given in K (Tmb).Kinstr.det.noisefloatnullableTmb? Main beam brightness peak intensity of the detected lineKobs.paramfloatnullableV0? Center velocity of the CO line (in km/s).km/sspect.dopplerVelocfloatnullablen_V0[ab] Remark on V0 (1)meta.notecharVexp? Expansion velocity. This is half of the full line width at zero intensity.km/sphys.veloc.expansionfloatnullableIco? CO intensity integrated over the whole line (in K.km/s, Tmb scale).K.km/sspect.line.intensityfloatnullableRef? Reference to a previous CO detection of the source. (2)meta.bibintnullableIdentSource name if differs from the IRAS name. An asterisk after the name indicates that there is an interstellar line included in the CO spectrum.meta.idcharSimbadSimbad column added by the CDSchar_RAPosition from IRAS-PSC (Cat. II/125) (right ascension part)degpos.eq.ra;meta.main_DEPosition from IRAS-PSC (Cat. II/125) (declination part)degpos.eq.dec;meta.mainJ/A+AS/93/121/table6Objects with cold envelopesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIRASIRAS Source Namemeta.id;meta.maincharRegionin the IRAS two color diagram as defined by van der Veen & Habing, 1988A&A...194..125Vobs.fieldcharDetDetection, as: D = Detected by us; ? = Tentative detection; N = Non-detection; * = Interstellar line in the CO spectrum.meta.codecharr_Det? Reference to previous detection (1)meta.ref;pos.frameintnullableIdentIdentificationmeta.idcharSpTypeMK spectral typesrc.spTypecharr_IdReference to Identification (1)meta.ref;pos.framechar