[DJW84] W49 G5 , the SIMBAD biblio

[DJW84] W49 G5 , the SIMBAD biblio (13 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST04:15:31


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Title First 3 Authors
1997ApJ...482..307D 49 92 Multifrequency, high-resolution radio recombination line observations of the massive star-forming region W49A. DE PREE C.G., MEHRINGER D.M. and GOSS W.M.
1999PASP..111.1049G 128 313 Massive stars: their environment and formation. (Invited review). GARAY G. and LIZANO S.
2000ApJ...540..308D 35 38 Ultracompact H II regions in W49N at 500 AU scales: shells, winds, and the water maser source. DE PREE C.G., WILNER D.J., GOSS W.M., et al.
2004ApJ...600..286D 19 16 Broad recombination line objects in W49 north on 600 AU scales. DE PREE C.G., WILNER D.J., MERCER A.J., et al.
2004MNRAS.347.1164P 28 11 VLA observations of 6-cm excited OH. PALMER P., GOSS W.M. and WHITEOAK J.B.
2005MNRAS.360..993P 24 1 Very Large Array observations of broad 6-cm excited-state OH lines in W49A. PALMER P. and GOSS W.M.
2006ApJ...653..409T 41 15 Hard X-rays from ultracompact H II regions in W49A. TSUJIMOTO M., HOSOKAWA T., FEIGELSON E.D., et al.
2009MNRAS.399..952S 189           X   F     4 33 9 Massive star formation and feedback in W49A: the source of our galaxy's most luminous water maser outflow. SMITH N., WHITNEY B.A., CONTI P.S., et al.
2015ApJ...810..147L 119           X         3 18 4 Extremely energetic outflow and decelerated expansion in W49N. LIU T., KIM K.-T., WU Y., et al.
2018ApJ...863L...9D 165           X C       3 27 1 Flux density variations at 3.6 cm in the massive star-forming region W49A. DE PREE C.G., GALVAN-MADRID R., GOSS W.M., et al.
2020AJ....160..234D 102       D     X         3 44 ~ Time-variable radio recombination line emission in W49A. DE PREE C.G., WILNER D.J., KRISTENSEN L.E., et al.
2021ApJ...923..198D 627       D     X C       14 62 3 Surveying the Giant H II regions of the Milky Way with SOFIA. III. W49A. DE BUIZER J.M., LIM W., LIU M., et al.
2022PASJ...74..128M 45           X         1 25 2 Star burst in W 49 N presumably induced by cloud-cloud collision. MIYAWAKI R., HAYASHI M. and HASEGAWA T.

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