Cl* NGC 6618 B 331 , the SIMBAD biblio

Cl* NGC 6618 B 331 , the SIMBAD biblio (24 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST13:24:26


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Title First 3 Authors
1984A&A...136...53F 35 135 A high resolution study of M 17 at 1.3, 2, 6 and 21 cm. FELLI M., CHURCHWELL E. and MASSI M.
1993MNRAS.264.1025H 7 21 High-resolution millimetre and submillimetre continuum observations of M 17SW - II. Identification of embedded sources associated with H2O masers. HOBSON M.P., PADMAN R., SCOTT P.F., et al.
1994Ap&SS.216..159H 5 1 The structure and dynamics of M17SW. HOBSON M.P.
1997ApJ...489..698H 326 220 The young massive stellar objects of M17. HANSON M.M., HOWARTH I.D. and CONTI P.S.
1998A&A...329..161C 70 39 Young stellar objects and abnormal extinction within M17. CHINI R. and WARGAU W.F.
2001A&A...377..273N 42 43 High mass Class I sources in M 17. NIELBOCK M., CHINI R., JUETTE M., et al.
2002AJ....124.1636K 13 11 Mid-infrared observations of M17. KASSIS M., DEUTSCH L.K., CAMPBELL M.F., et al.
2003ApJ...593..874T 130 196 10 MK gas in M17 and the Rosette nebula: X-ray flows in galactic H II regions. TOWNSLEY L.K., FEIGELSON E.D., MONTMERLE T., et al.
2006A&A...457L..29H         O           14 15 2.3 µm CO emission and absorption from young high-mass stars in M 17. HOFFMEISTER V.H., CHINI R., SCHEYDA C.M., et al.
2006A&A...457.1081K 91 120 A catalogue of Galactic supernova remnants from the Canadian Galactic plane survey. I. Flux densities, spectra, and polarization characteristics. KOTHES R., FEDOTOV K., FOSTER T.J., et al.
2007ApJS..169..353B viz 934 123 The young stellar population in M17 revealed by Chandra. BROOS P.S., FEIGELSON E.D., TOWNSLEY L.K., et al.
2008ApJ...686..310H 52       D     X         2 61 87 The stellar population of M17. HOFFMEISTER V.H., CHINI R., SCHEYDA C.M., et al.
2012ApJ...755..152R 15       D               2 47 20 Compact radio sources in M17. RODRIGUEZ L.F., GONZALEZ R.F., MONTES G., et al.
2017A&A...599L...9S 79           X         2 26 10 A dearth of short-period massive binaries in the young massive star forming region M 17. Evidence for a large orbital separation at birth? SANA H., RAMIREZ-TANNUS M.C., DE KOTER A., et al.
2017ApJ...838...61P viz 16       D               1 492 4 Candidate X-ray OB stars in MYStIX massive star-forming regions. POVICH M.S., BUSK H.A., FEIGELSON E.D., et al.
2017A&A...604A..78R viz 1350           X C       33 19 21 Massive pre-main-sequence stars in M17. RAMIREZ-TANNUS M.C., KAPER L., DE KOTER A., et al.
2018A&A...620A..52R viz 337       D     X         9 27 4 Diffuse interstellar bands in the H II region M17. Insights into their relation with the total-to-selective visual extinction RV. RAMIREZ-TANNUS M.C., COX N.L.J., KAPER L., et al.
2020ApJ...888...98L 1210       D S   X C       28 45 15 Surveying the giant H II regions of the Milky Way with SOFIA. II. M17. LIM W., DE BUIZER J.M. and RADOMSKI J.T.
2022ApJ...929...27H 171           X C       3 9 12 Studying Magnetic Fields and Dust in M17 Using Polarized Thermal Dust Emission Observed by SOFIA/HAWC+. HOANG T.D., NGOC N.B., DIEP P.N., et al.
2023A&A...671A..13B 3308     A D S   X C       75 13 1 Massive pre-main-sequence stars in M17 Modelling hydrogen and dust in MYSO disks. BACKS F., POORTA J., RAB C., et al.
2023A&A...676A.122P 1628       D     X C       37 11 ~ Massive pre-main-sequence stars in M17 First and second overtone CO bandhead emission and the thermal infrared. POORTA J., RAMIREZ-TANNUS M.C., DE KOTER A., et al.
2024A&A...690A.178R viz 332       D     X C       7 41 ~ The spectroscopic binary fraction of the young stellar cluster M17. RAMIREZ-TANNUS M.C., DERKINK A.R., BACKS F., et al.
2025A&A...694A.295P 3219     A D     X C       69 15 ~ ALMA detections of circumstellar disks in the giant H II region M17 Probing the intermediate- to high-mass pre-main-sequence population. POORTA J., HOGERHEIJDE M., DE KOTER A., et al.
2025MNRAS.538.2392M 19       D               1 7 ~ Strengthening the link between fullerenes and a subset of diffuse interstellar bands. MAJAESS D., HARRIOTT T.A., SEURET H., et al.

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