NAME 1.5 Complex , the SIMBAD biblio

NAME 1.5 Complex , the SIMBAD biblio (15 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST08:19:15


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Title First 3 Authors
1988ApJ...324..223B 5 13 304 Galactic Center molecular clouds. II. Distribution and kinematics. BALLY J., STARK A.A., WILSON R.W., et al.
2010ApJ...721..137B viz 267           X C       6 1519 106 The Bolocam Galactic Plane Survey: λ = 1.1 and 0.35 mm dust continuum emission in the Galactic Center region. BALLY J., AGUIRRE J., BATTERSBY C., et al.
2010A&A...523A..45R 1236       D S   X C       31 20 32 A survey of the Galactic Center region in HCO+, H13CO+, and SiO. RIQUELME D., BRONFMAN L., MAUERSBERGER R., et al.
2011ApJ...735...19S 177     A     X C       4 29 57 Star-forming c
loud comp
lexes in the centra
l mo
lecu
lar zone of NGC 253.
SAKAMOTO K., MAO R.-Q., MATSUSHITA S., et al.
2013A&A...549A..36R 94       D     X         3 8 9 Kinetic temperatures toward X1/X2 orbit interceptions regions and giant molecular loops in the Galactic Center region. RIQUELME D., AMO-BALADRON M.A., MARTIN-PINTADO J., et al.
2014MNRAS.440.3370K 498       D     X C       12 11 224 What controls star formation in the central 500 pc of the Galaxy ? KRUIJSSEN J.M.D., LONGMORE S.N., ELMEGREEN B.G., et al.
2015ApJS..219...28Z viz 794     A D     X         21 10 3 Isotopic ratios of 18O/17O in the galactic central region. ZHANG J.S., SUN L.L., RIQUELME D., et al.
2015MNRAS.454.3049S 40           X         1 5 8 Stochastic non-circular motion and outflows driven by magnetic activity in the Galactic bulge region. SUZUKI T.K., FUKUI Y., TORII K., et al.
2017MNRAS.467.4622J 41           X         1 10 4 Does the SN rate explain the very high energy cosmic rays in the central 200 pc of our Galaxy? JOUVIN L., LEMIERE A. and TERRIER R.
2018ApJS..234...22P viz 346       D     X C       8 2382 33 The dusty Galactic Center as seen by SCUBA-2. PARSONS H., DEMPSEY J.T., THOMAS H.S., et al.
2020ApJS..249....6Z viz 85             C       1 31 9 A systematic observational study on Galactic interstellar ratio 18O/17O. I. C18O and C17O J = 1-0 data analysis. ZHANG J.S., LIU W., YAN Y.T., et al.
2020MNRAS.499.4455T 329     A S   X         7 11 64 Simulations of the Milky Way's central molecular zone - I. Gas dynamics. TRESS R.G., SORMANI M.C., GLOVER S.C.O., et al.
2021ApJ...920....6G 218       S   X         4 18 11 The Atacama Cosmology Telescope: microwave intensity and polarization maps of the Galactic Center. GUAN Y., CLARK S.E., HENSLEY B.S., et al.
2022A&A...668A.183B viz 5241 T   A D S   X C       115 13 ~ Living on the edge of the Milky Way's central molecular zone
G1.3 is the more likely candidate for gas accretion into the CMZ.
BUSCH L.A., RIQUELME D., GUSTEN R., et al.
2023ApJ...959...93G 233           X C       4 8 ~ Evidence of a Cloud-Cloud Collision from Overshooting Gas in the Galactic Center. GRAMZE S.R., GINSBURG A., MEIER D.S., et al.

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