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2023A&A...674A..40G - Astronomy and Astrophysics, volume 674A40 (2023/6-1)
Gaia Data Release 3 Exploring and mapping the diffuse interstellar band at 862 nm.
GAIA COLLABORATION, SCHULTHEIS M., ZHAO H., ZWITTER T., MARSHALL D.J., DRIMMEL R., FREMAT Y., BAILER-JONES C.A.L., RECIO-BLANCO A., KORDOPATIS G., DE LAVERNY P., ANDRAE R., DHARMAWARDENA T.E., FOUESNEAU M., SORDO R., BROWN A.G.A., VALLENARI A., PRUSTI T., DE BRUIJNE J.H.J., ARENOU F., BABUSIAUX C., BIERMANN M., CREEVEY O.L., DUCOURANT C., EVANS D.W., EYER L., GUERRA R., HUTTON A., JORDI C., KLIONER S.A., LAMMERS U.L., LINDEGREN L., LURI X., MIGNARD F., PANEM C., POURBAIX D., RANDICH S., SARTORETTI P., SOUBIRAN C., TANGA P., WALTON N.A., BASTIAN U., JANSEN F., KATZ D., LATTANZI M.G., VAN LEEUWEN F., BAKKER J., CACCIARI C., CASTANEDA J., DE ANGELI F., FABRICIUS C., GALLUCCIO L., GUERRIER A., HEITER U., MASANA E., MESSINEO R., MOWLAVI N., NICOLAS C., NIENARTOWICZ K., PAILLER F., PANUZZO P., RICLET F., ROUX W., SEABROKE G.M., THEVENIN F., GRACIA-ABRIL G., PORTELL J., TEYSSIER D., ALTMANN M., AUDARD M., BELLAS-VELIDIS I., BENSON K., BERTHIER J., BLOMME R., BURGESS P.W., BUSONERO D., BUSSO G., CANOVAS H., CARRY B., CELLINO A., CHEEK N., CLEMENTINI G., DAMERDJI Y., DAVIDSON M., DE TEODORO P., NUNEZ CAMPOS M., DELCHAMBRE L., DELL'ORO A., ESQUEJ P., FERNANDEZ-HERNANDEZ J., FRAILE E., GARABATO D., GARCIA-LARIO P., GOSSET E., HAIGRON R., HALBWACHS J.-L., HAMBLY N.C., HARRISON D.L., HERNANDEZ J., HESTROFFER D., HODGKIN S.T., HOLL B., JANSSEN K., JEVARDAT DE FOMBELLE G., JORDAN S., KRONE-MARTINS A., LANZAFAME A.C., LOFFLER W., MARCHAL O., MARRESE P.M., MOITINHO A., MUINONEN K., OSBORNE P., PANCINO E., PAUWELS T., REYLE C., RIELLO M., RIMOLDINI L., ROEGIERS T., RYBIZKI J., SARRO L.M., SIOPIS C., SMITH M., SOZZETTI A., UTRILLA E., VAN LEEUWEN M., ABBAS U., ABRAHAM P., ABREU ARAMBURU A., AERTS C., AGUADO J.J., AJAJ M., ALDEA-MONTERO F., ALTAVILLA G., ALVAREZ M.A., ALVES J., ANDERS F., ANDERSON R.I., ANGLADA VARELA E., ANTOJA T., BAINES D., BAKER S.G., BALAGUER-NUNEZ L., BALBINOT E., BALOG Z., BARACHE C., BARBATO D., BARROS M., BARSTOW M.A., BARTOLOME S., BASSILANA J.-L., BAUCHET N., BECCIANI U., BELLAZZINI M., BERIHUETE A., BERNET M., BERTONE S., BIANCHI L., BINNENFELD A., BLANCO-CUARESMA S., BOCH T., BOMBRUN A., BOSSINI D., BOUQUILLON S., BRAGAGLIA A., BRAMANTE L., BREEDT E., BRESSAN A., BROUILLET N., BRUGALETTA E., BUCCIARELLI B., BURLACU A., BUTKEVICH A.G., BUZZI R., CAFFAU E., CANCELLIERE R., CANTAT-GAUDIN T., CARBALLO R., CARLUCCI T., CARNERERO M.I., CARRASCO J.M., CASAMIQUELA L., CASTELLANI M., CASTRO-GINARD A., CHAOUL L., CHARLOT P., CHEMIN L., CHIARAMIDA V., CHIAVASSA A., CHORNAY N., COMORETTO G., CONTURSI G., COOPER W.J., CORNEZ T., COWELL S., CRIFO F., CROPPER M., CROSTA M., CROWLEY C., DAFONTE C., DAPERGOLAS A., DAVID P., DE LUISE F., DE MARCH R., DE RIDDER J., DE SOUZA R., DE TORRES A., DEL PELOSO E.F., DEL POZO E., DELBO M., DELGADO A., DELISLE J.-B., DEMOUCHY C., DIAKITE S., DIENER C., DISTEFANO E., DOLDING C., ENKE H., FABRE C., FABRIZIO M., FAIGLER S., FEDORETS G., FERNIQUE P., FIGUERAS F., FOURNIER Y., FOURON C., FRAGKOUDI F., GAI M., GARCIA-GUTIERREZ A., GARCIA-REINALDOS M., GARCIA-TORRES M., GAROFALO A., GAVEL A., GAVRAS P., GERLACH E., GEYER R., GIACOBBE P., GILMORE G., GIRONA S., GIUFFRIDA G., GOMEL R., GOMEZ A., GONZALEZ-NUNEZ J., GONZALEZ-SANTAMARIA I., GONZALEZ-VIDAL J.J., GRANVIK M., GUILLOUT P., GUIRAUD J., GUTIERREZ-SANCHEZ R., GUY L.P., HATZIDIMITRIOU D., HAUSER M., HAYWOOD M., HELMER A., HELMI A., SARMIENTO M.H., HIDALGO S.L., HLADCZUK N., HOBBS D., HOLLAND G., HUCKLE H.E., JARDINE K., JASNIEWICZ G., JEAN-ANTOINE PICCOLO A., JIMENEZ-ARRANZ O., JUARISTI CAMPILLO J., JULBE F., KARBEVSKA L., KERVELLA P., KHANNA S., KORN A.J., KOSPAL A., KOSTRZEWA-RUTKOWSKA Z., KRUSZYNSKA K., KUN M., LAIZEAU P., LAMBERT S., LANZA A.F., LASNE Y., LE CAMPION J.-F., LEBRETON Y., LEBZELTER T., LECCIA S., LECLERC N., LECOEUR-TAIBI I., LIAO S., LICATA E.L., LINDSTROM H.E.P., LISTER T.A., LIVANOU E., LOBEL A., LORCA A., LOUP C., MADRERO PARDO P., MAGDALENO ROMEO A., MANAGAU S., MANN R.G., MANTEIGA M., MARCHANT J.M., MARCONI M., MARCOS J., MARCOS SANTOS M.M.S., MARIN PINA D., MARINONI S., MAROCCO F., MARTIN POLO L., MARTIN-FLEITAS J.M., MARTON G., MARY N., MASIP A., MASSARI D., MASTROBUONO-BATTISTI A., MAZEH T., McMILLAN P.J., MESSINA S., MICHALIK D., MILLAR N.R., MINTS A., MOLINA D., MOLINARO R., MOLNAR L., MONARI G., MONGUIO M., MONTEGRIFFO P., MONTERO A., MOR R., MORA A., MORBIDELLI R., MOREL T., MORRIS D., MURAVEVA T., MURPHY C.P., MUSELLA I., NAGY Z., NOVAL L., OCANA F., OGDEN A., ORDENOVIC C., OSINDE J.O., PAGANI C., PAGANO I., PALAVERSA L., PALICIO P.A., PALLAS-QUINTELA L., PANAHI A., PAYNE-WARDENAAR S., PENALOSA ESTELLER X., PENTTILA A., PICHON B., PIERSIMONI A.M., PINEAU F.-X., PLACHY E., PLUM G., POGGIO E., PRSA A., PULONE L., RACERO E., RAGAINI S., RAINER M., RAITERI C.M., RAMOS P., RAMOS-LERATE M., RE FIORENTIN P., REGIBO S., RICHARDS P.J., RIOS DIAZ C., RIPEPI V., RIVA A., RIX H.-W., RIXON G., ROBICHON N., ROBIN A.C., ROBIN C., ROELENS M., ROGUES H.R.O., ROHRBASSER L., ROMERO-GOMEZ M., ROWELL N., ROYER F., RUZ MIERES D., RYBICKI K.A., SADOWSKI G., SAEZ NUNEZ A., SAGRISTA SELLES A., SAHLMANN J., SALGUERO E., SAMARAS N., SANCHEZ GIMENEZ V., SANNA N., SANTOVENA R., SARASSO M., SCIACCA E., SEGOL M., SEGOVIA J.C., SEGRANSAN D., SEMEUX D., SHAHAF S., SIDDIQUI H.I., SIEBERT A., SILTALA L., SILVELO A., SLEZAK E., SLEZAK I., SMART R.L., SNAITH O.N., SOLANO E., SOLITRO F., SOUAMI D., SOUCHAY J., SPAGNA A., SPINA L., SPOTO F., STEELE I.A., STEIDELMULLER H., STEPHENSON C.A., SUVEGES M., SURDEJ J., SZABADOS L., SZEGEDI-ELEK E., TARIS F., TAYLOR M.B., TEIXEIRA R., TOLOMEI L., TONELLO N., TORRA F., TORRA J., TORRALBA ELIPE G., TRABUCCHI M., TSOUNIS A.T., TURON C., ULLA A., UNGER N., VAILLANT M.V., VAN DILLEN E., VAN REEVEN W., VANEL O., VECCHIATO A., VIALA Y., VICENTE D., VOUTSINAS S., WEILER M., WEVERS T., WYRZYKOWSKI L., YOLDAS A., YVARD P., ZOREC J. and ZUCKER S.
Abstract (from CDS):
Aims. Here, we demonstrate the capacity of the Gaia-Radial Velocity Spectrometer (RVS) in Gaia DR3 to reveal the spatial distribution of the unknown molecular species responsible for the most prominent DIB at 862 nm in the RVS passband, exploring the Galactic ISM within a few kiloparsecs from the Sun.
Methods. The DIBs are measured within the GSP-Spec module using a Gaussian profile fit for cool stars and a Gaussian process for hot stars. In addition to the equivalent widths and their uncertainties, Gaia DR3 provides their characteristic central wavelength, width, and quality flags.
Results. We present an extensive sample of 476 117 individual DIB measurements obtained in a homogeneous way covering the entire sky. We compare spatial distributions of the DIB carrier with interstellar reddening and find evidence that DIB carriers are present in a local bubble around the Sun which contains nearly no dust. We characterised the DIB equivalent width with a local density of 0.19 ± 0.04 Å kpc–1 and a scale height of $ 98.60_{-8.46}^{+11.10} $ pc. The latter is smaller than the dust scale height, indicating that DIBs are more concentrated towards the Galactic plane. We determine the rest-frame wavelength with unprecedented precision (λ0 = 8620.86 ± 0.019 Å in air) and reveal a remarkable correspondence between the DIB velocities and the CO gas velocities, suggesting that the 862 nm DIB carrier is related to macro-molecules.
Conclusions. We demonstrate the unique capacity of Gaia to trace the spatial structure of the Galactic ISM using the 862 nm DIB.
Abstract Copyright: © The Authors 2023
Journal keyword(s): ISM: lines and bands - ISM: kinematics and dynamics - dust, extinction
Simbad objects: 33
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