LDN 1188 , the SIMBAD biblio

LDN 1188 , the SIMBAD biblio (24 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST03:47:37

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
1962ApJS....7....1L viz 1829 890 Catalogue of dark nebulae. LYNDS B.T.
1995A&A...300..525A 106 T K                 40 9 Molecular material and young stellar objects in the
L 1188 dark cloud complex. 		ABRAHAM P., DOBASHI K., MIZUNO A., et al.
1997ApJS..110...21Y viz 396 149 Molecular clouds in Cepheus and Cassiopeia. YONEKURA Y., DOBASHI K., MIZUNO A., et al.
1999A&AS..134..241P viz 124 34 Rotation in molecular clouds. PHILLIPS J.P.
2002A&A...383..631D viz 14       D               3330 41 A catalogue of dust clouds in the Galaxy. DUTRA C.M. and BICA E.
2004A&A...418..131K viz 913 29 Far-infrared loops in the 2nd Galactic Quadrant. KISS C., MOOR A. and TOTH L.V.
2004BaltA..13..470K 110 T K                 10 3 Young objects in
L 1188. 		KOENYVES V., MOOR A., KISS C., et al.
2005MNRAS.362..753D 5 32 481 The INT Photometric Hα Survey of the Northern Galactic Plane (IPHAS). DREW J.E., GREIMEL R., IRWIN M.J., et al.
2005PASJ...57S...1D viz 15       D               5394 307 Atlas and catalog of dark clouds based on Digitized Sky Survey I. DOBASHI K., UEHARA H., KANDORI R., et al.
2017ApJ...835L..14G 1311 T         X C       31 12 19
L1188: a promising candidate for cloud-cloud collisions triggering the formation of low- and intermediate-mass stars. 		GONG Y., FANG M., MAO R., et al.
2017MNRAS.466.1082J 40           X         1 24 7 Q+: characterizing the structure of young star clusters. JAFFA S.E., WHITWORTH A.P. and LOMAX O.
2018MNRAS.477..977Z 104     A     X         3 6 2 IRAS 22150+6109 - a young B-type star with a large disc. ZAKHOZHAY O.V., MIROSHNICHENKO A.S., KURATOV K.S., et al.
2019ApJ...871...44T 41           X         1 62 40 Formation of the active star-forming region LHA 120-N 44 triggered by tidally driven colliding H I flows. TSUGE K., SANO H., TACHIHARA K., et al.
2018PASJ...70S..41F 41           X         1 44 45 Molecular clouds in the NGC 6334 and NGC 6357 region: Evidence for a 100 pc-scale cloud-cloud collision triggering the Galactic mini-starbursts. FUKUI Y., KOHNO M., YOKOYAMA K., et al.
2018PASJ...70S..45O 40           X         1 30 19 The formation of a Spitzer bubble RCW 79 triggered by a cloud-cloud collision. OHAMA A., KOHNO M., HASEGAWA K., et al.
2018PASJ...70S..50K 40           X         1 67 36 FOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45 m telescope (FUGIN): Molecular clouds toward W 33; possible evidence for a cloud-cloud collision triggering O star formation. KOHNO M., TORII K., TACHIHARA K., et al.
2019MNRAS.484.1800S 5401 T K A D S   X C F     130 154 2 The young star population of
Lynds 1188. 		SZEGEDI-ELEK E., KUN M., MOOR A., et al.
2019A&A...632A.115G viz 1324 T K A S   X C       30 15 ~ Searching for further evidence for cloud-cloud collisions in
L1188. 		GONG Y., TANG X.D., HENKEL C., et al.
2020ApJ...893L...5X 82           X         2 6 ~ First embedded cluster formation in California Molecular Cloud. XU J.-L., XU Y., JIANG P., et al.
2020MNRAS.499.3620I 82           X         2 4 ~ G133.50+9.01: a likely cloud-cloud collision complex triggering the formation of filaments, cores, and a stellar cluster. ISSAC N., TEJ A., LIU T., et al.
2021ApJS..254....3M viz 84           X         2 17 11 Molecular clouds in the second quadrant of the Milky Way midplane from l = 104.75° to l = 119.75° and b = -5.25° to b = 5.25°. MA Y., WANG H., LI C., et al.
2023MNRAS.521..354W viz 44           X         1 53 ~ A naive Bayes classifier for identifying Class II YSOs. WILSON A.J., LAKELAND B.S., WILSON T.J., et al.
2023MNRAS.520.1390S viz 496       D     X C       11 926 1 The Gaia view of the Cepheus OB2 association. SZILAGYI M., KUN M., ABRAHAM P., et al.
2024MNRAS.527.4297C 45           X         1 34 ~ Cloud-cloud collision in S235: triggered the formation of high-mass stars and young star clusters. CHEN E., GAO Y., ZHANG S., et al.

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