MBM 16 , the SIMBAD biblio

MBM 16 , the SIMBAD biblio (63 results) C.D.S. - SIMBAD4 rel 1.8 - 2023.04.02CEST13:43:43


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Title First 3 Authors
1985ApJ...295..402M 124 434 Molecular gas at high galactic latitudes. MAGNANI L., BLITZ L. and MUNDY L.
1988ApJ...326..909M 18 71 Molecular abundances in the high-latitude molecular clouds. MAGNANI L., BLITZ L. and WOUTERLOOT J.G.A.
1988ApJ...327..356H 35   K                 24 69 On the nearest molecular clouds. II. MBM 12 and 16. HOBBS L.M., BLITZ L., PENPRASE B.E., et al.
1988ApJ...331L.127B 1 6 31 Broad-wing molecular lines without internal energy sources. BLITZ L., MAGNANI L. and WANDEL A.
1989AJ.....98..926M 12 12 A search for SH+ and CH+ in diffuse and translucent clouds. MAGNANI L. and SALZER J.J.
1989ApJ...339..244M 13 22 CH observations of diffuse molecular clouds. MAGNANI L., LADA E.A., SANDELL G., et al.
1989ApJ...344..292T 17 50 On the nature of the molecular cores in high-latitude cirrus clouds. I. A survey of H2CO (2 centimeter), C3H2 and HC3N. TURNER B.E., RICKARD L.J. and XU L.-P.
1989ApJ...346..232W 32 42 On the nearest molecular clouds. III. MBM 40, 53, 54 and 55. WELTY D.E., HOBBS L.M., BLITZ L., et al.
1990ApJ...359..344F 3 13 160 A signature of the intermittency of interstellar turbulence: the wings of molecular line profiles. FALGARONE E. and PHILLIPS T.G.
1990ApJ...359..355M 9 20 Hydroxyl emission in translucent molecular clouds. MAGNANI L. and SISKIND L.
1990ApJS...73..747M 1 3 15 Structure in small molecular clouds: pedestals and clumping. MAGNANI L., CARPENTER J.M., BLITZ L., et al.
1992BAAS...24.1164L 1 ~ The observation of coherent velocity structures in a translucent molecular cloud and implications for turbulence. LAROSA T.N., MAGNANI L. and SHORE S.
1992BAAS...24.1199M 1 ~ High resolution H2CO observations of correlated velocity structure in a translucent molecular cloud. MAGNANI L., et al.
1993ApJ...402..226M 36   K                 5 28 The observation of correlated velocity structures in a translucent molecular cloud and implications for turbulence. MAGNANI L., LAROSA T.N. and SHORE S.N.
1994ApJ...434..162G 18 39 The association of high-latitude molecular clouds with H I gas. GIR B.-Y., BLITZ L. and MAGNANI L.
1995A&A...300..903B 1 15 89 The Orion OB1 association. II. The Orion-Eridanus Bubble. BROWN A.G.A., HARTMANN D. and BURTON W.B.
1995ApJ...443..169M 35 45 A new method for determining the CO to H2 conversion factor for translucent clouds. MAGNANI L. and ONELLO J.S.
1996ApJS..106..447M 121 65 A catalog of molecular gas at high galactic latitudes. MAGNANI L., HARTMANN D. and SPECK B.G.
1997A&A...325..647N viz 125 76 Optical high-resolution spectroscopy of ROSAT detected late-type stars south of the Taurus molecular clouds. NEUHAEUSER R., TORRES G., STERZIK M.F., et al.
1997ApJ...476..717G 18 10 The structure of the galactic magnetic field toward the high-latitude clouds. GOMEZ DE CASTRO A.I., PUDRITZ R.E. and BASTIEN P.
1997ApJ...484..245K 10 28 X-ray shadows by high-latitude molecular clouds. I. Cartography. KUNTZ K.D., SNOWDEN S.L. and VERTER F.
1998AJ....115..745V 11 10 Infrared properties of molecular cirrus. I. Photometry of extended sources on IRAS image products. VERTER F. and RICKARD L.J.
1998ApJ...504..290M 14 24 The variation of the CO to H2 conversion factor in two translucent clouds. MAGNANI L., ONELLO J.S., ADAMS N.G., et al.
1998ApJ...507..507R 152 68 Infrared excess and molecular clouds: a comparison of new surveys of far-infrared and H I 21 centimeter emission at high galactic latitudes. REACH W.T., WALL W.F. and ODEGARD N.
1999A&A...347..640B 1 23 101 PRONAOS observations of MCLD 123.5+24.9: cold dust in the Polaris cirrus cloud. BERNARD J.P., ABERGEL A., RISTORCELLI I., et al.
1999ApJ...512..761L 114 T K                 1 16 A dynamical study of the non-star-forming translucent molecular cloud
MBM 16: evidence for shear-driven turbulence in the interstellar medium.
LAROSA T.N., SHORE S.N. and MAGNANI L.
1999Ap.....42..234N 18 0 T associations in X-rays. NEUHAEUSER R. and HAMBARYAN V.
2000A&A...356..157L 65 16 New discovery of weak-line T Tauri stars in high-Galactic latitude molecular clouds. LI J.Z., HU J.Y. and CHEN W.P.
2000ApJ...535..167M 34 37 A survey of high-latitude molecular gas in the southern galactic hemisphere. MAGNANI L., HARTMANN D., HOLCOMB S.L., et al.
2000ApJ...536..831V 16 11 Infrared properties of molecular cirrus. II. Cloud-to-Cloud variations in graphite and polycyclic aromatic hydrocarbon content. VERTER F., MAGNANI L., DWEK E., et al.
2002A&A...391..693L 28 35 Comparative chemistry of diffuse clouds. IV: CH. LISZT H. and LUCAS R.
2003A&A...411..447L viz 571 216 3D mapping of the dense interstellar gas around the Local Bubble. LALLEMENT R., WELSH B.Y., VERGELY J.-L., et al.
2003ApJ...586.1111M 6 1 20 CH, CO, and E(B-V) as molecular gas tracers in a translucent cloud. MAGNANI L., CHASTAIN R.J., KIM H.C., et al.
2003ApJ...593..413S 9 9 Mechanisms for the origin of turbulence in non-star-forming clouds: the translucent cloud MBM 40. SHORE S.N., MAGNANI L., LAROSA T.N., et al.
2003ApJ...595..858L 45 82 Far Ultraviolet Spectroscopic Explorer survey of the local interstellar medium within 200 parsecs. LEHNER N., JENKINS E.B., GRY C., et al.
2005AJ....130.2725M 5 7 CH 3 GHz observations of molecular clouds along the galactic plane. MAGNANI L., LUGO S. and DAME T.M.
2006A&A...457..197S 5 5 Random flows and diagnostics of turbulence in the high latitude cirrus. SHORE S.N., LAROSA T.N., CHASTAIN R.J., et al.
2006AJ....132.1964C 15 4 A high-latitude molecular structure in Pegasus-Pisces. CHASTAIN R.J., SHELTON R.L., RALEY E.A., et al.
2007ApJ...654L.131M 23 18 Galactic dust clouds are shining in scattered Hα light. MATTILA K., JUVELA M. and LEHTINEN K.
1993ApJ...408..559M 38   K                 1 12 CH as a tracer of a translucent cloud boundary. MAGNANI L. and ONELLO J.S.
2010AJ....139..267C 922           X         24 8 8 High-resolution CH observations of two translucent molecular clouds. CHASTAIN R.J., COTTEN D. and MAGNANI L.
2010A&A...512A..67L 192           X C       4 59 87 2MASS wide field extinction maps. III. The Taurus, Perseus, and California cloud complexes. LOMBARDI M., LADA C.J. and ALVES J.
2012A&A...547A..85B viz 195           X C       4 23 0 Molecular gas and stars in the translucent cloud MBM 18 (LDN 1569). BRAND J., WOUTERLOOT J.G.A. and MAGNANI L.
2013ApJ...779...36P 1519 T   A     X C       37 9 8 Characterizing the turbulent properties of the starless molecular cloud
MBM 16.
PINGEL N.M., STANIMIROVIC S., PEEK J.E.G., et al.
2013MNRAS.436.1152C 80           X         2 3 8 A high-resolution study of the CO-H2 conversion factor in the diffuse cloud MBM 40. COTTEN D.L. and MAGNANI L.
2014ApJ...786...29S viz 56       D     X         2 89 102 A large catalog of accurate distances to molecular clouds from PS1 photometry. SCHLAFLY E.F., GREEN G., FINKBEINER D.P., et al.
2015ApJ...808...22H 1381       D     X C       34 11 8 XMM-Newton and Suzaku X-ray shadowing measurements of the solar wind charge exchange, Local Bubble, and galactic halo emission. HENLEY D.B. and SHELTON R.L.
2016ApJ...816...82L 934 T   A D     X C       22 5 1 Evidence for a very low-column density hole in the galactic halo in the direction of the high latitude molecular cloud
MBM 16.
LIU W., GALEAZZI M. and URSINO E.
2017ApJ...845...53N 123           X         3 5 2 Spatial variations of turbulent properties of neutral hydrogen gas in the Small Magellanic Cloud using structure-function analysis. NESTINGEN-PALM D., STANIMIROVIC S., GONZALEZ-CASANOVA D.F., et al.
2017A&A...607A..15K 1399       S   X C       32 7 5 H I anisotropies associated with radio-polarimetric filaments. Steep power spectra associated with cold gas. KALBERLA P.M.W., KERP J., HAUD U., et al.
2018ApJS..234....2P viz 42           X         1 9 8 The GALFA-HI survey data release 2. PEEK J.E.G., BABLER B.L., ZHENG Y., et al.
2018ApJ...856..136P 59       D     X         2 14 1 Multi-phase turbulence density power spectra in the Perseus molecular cloud. PINGEL N.M., LEE M.-Y., BURKHART B., et al.
2018A&A...611A..51R 42           X         1 16 3 Cosmic-rays, gas, and dust in nearby anticentre clouds. II. Interstellar phase transitions and the dark neutral medium. REMY Q., GRENIER I.A., MARSHALL D.J., et al.
2018ApJ...862...34N viz 59       D     X         2 9 ~ Spatial distribution of the Milky Way hot gaseous halo constrained by Suzaku X-ray observations. NAKASHIMA S., INOUE Y., YAMASAKI N., et al.
2019A&A...623A..68T 43           X         1 16 ~ Small-scale physical and chemical structure of diffuse and translucent molecular clouds along the line of sight to Sgr B2. THIEL V., BELLOCHE A., MENTEN K.M., et al.
2019ApJ...879..125Z 17       D               1 100 ~ A large catalog of accurate distances to local molecular clouds: the Gaia DR2 edition. ZUCKER C., SPEAGLE J.S., SCHLAFLY E.F., et al.
2019A&A...631A..52J 128           X         3 33 ~ Gas shells and magnetic fields in the Orion-Eridanus superbubble. JOUBAUD T., GRENIER I.A., BALLET J., et al.
2021A&A...653A..63S 18       D               2 81 ~ Bird's eye view of molecular clouds in the Milky Way. I. Column density and star formation from sub-parsec to kiloparsec scales. SPILKER A., KAINULAINEN J. and ORKISZ J.
2021ApJS..256...46S viz 18       D               1 87 ~ The extinction and distance of the MBM molecular clouds at high galactic latitude. SUN M., JIANG B., ZHAO H., et al.
2021PASP..133j2001B 18       D               1 11 ~ Diagnosing turbulence in the neutral and molecular interstellar medium of galaxies. BURKHART B.
2021ApJ...920..103X 90           X         2 27 ~ Planck Galactic Cold Clumps at high Galactic latitude-a study with CO lines. XU F., WU Y., LIU T., et al.
2022ApJ...926..190R 140           X         3 11 ~ The Role of Neutral Hydrogen in Setting the Abundances of Molecular Species in the Milky Way's Diffuse Interstellar Medium. II. Comparison between Observations and Theoretical Models. RYBARCZYK D.R., GONG M., STANIMIROVIC S., et al.
2022PASJ...74.1396U 19       D               1 89 ~ The soft X-ray background with Suzaku. I. Milky Way halo. UEDA M., SUGIYAMA H., KOBAYASHI S.B., et al.

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2023.04.02-13:43:43

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