[DB2002b] G145.96-49.08 , the SIMBAD biblio

[DB2002b] G145.96-49.08 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST13:51:44


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Title First 3 Authors
1985ApJ...295..402M 124 485 Molecular gas at high galactic latitudes. MAGNANI L., BLITZ L. and MUNDY L.
1996ApJS..106..447M 121 77 A catalog of molecular gas at high galactic latitudes. MAGNANI L., HARTMANN D. and SPECK B.G.
1998ApJ...507..507R 152 83 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.
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...383..631D viz 15       D               3330 41 A catalogue of dust clouds in the Galaxy. DUTRA C.M. and BICA E.
2006AJ....132.1964C 15 4 A high-latitude molecular structure in Pegasus-Pisces. CHASTAIN R.J., SHELTON R.L., RALEY E.A., et al.
2014ApJ...786...29S viz 16       D               1 89 166 A large catalog of accurate distances to molecular clouds from PS1 photometry. SCHLAFLY E.F., GREEN G., FINKBEINER D.P., et al.
2014ApJ...786...97H viz 16       D               1 329 295 An optical spectroscopic study of T Tauri stars. I. Photospheric properties. HERCZEG G.J. and HILLENBRAND L.A.
2019A&A...624A...6Y 84             C       1 53 35 Distances to molecular clouds at high galactic latitudes based on Gaia DR2. YAN Q.-Z., ZHANG B., XU Y., et al.
2019ApJ...879..125Z 18       D               1 100 171 A large catalog of accurate distances to local molecular clouds: the Gaia DR2 edition. ZUCKER C., SPEAGLE J.S., SCHLAFLY E.F., et al.
2021ApJS..256...46S viz 366       D     X C       8 87 7 The extinction and distance of the MBM molecular clouds at high galactic latitude. SUN M., JIANG B., ZHAO H., et al.

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