The Proper Motion of Pyxis: The First Use of Adaptive Optics in Tandem with HST on a Faint Halo Object
![How to Constrain Your M Dwarf. II. The Mass–Luminosity–Metallicity Relation from 0.075 to 0.70 Solar Masses - IOPscience How to Constrain Your M Dwarf. II. The Mass–Luminosity–Metallicity Relation from 0.075 to 0.70 Solar Masses - IOPscience](https://cfn-live-content-bucket-iop-org.s3.amazonaws.com/journals/0004-637X/871/1/63/revision1/apjaaf3bcf8_hr.jpg?AWSAccessKeyId=AKIAYDKQL6LTV7YY2HIK&Expires=1677713881&Signature=%2Fw6WHHUuyt1MoLo1MNUZ%2BVUgrkE%3D)
How to Constrain Your M Dwarf. II. The Mass–Luminosity–Metallicity Relation from 0.075 to 0.70 Solar Masses - IOPscience
The MBHBM⋆ Project – I: Measurement of the Central Black Hole Mass in Spiral Galaxy NGC 3504 Using Molecular Gas Kinematics
The fossil record of two-phase galaxy assembly: Kinematics and metallicities in the nearest S0 galaxy
Click on the WR icon to view a course outline. Click on the Copy icon to copy a course to edit. Click More for Guidelines on Cou
![The Disc Origin of the Milky Way Bulge | Publications of the Astronomical Society of Australia | Cambridge Core The Disc Origin of the Milky Way Bulge | Publications of the Astronomical Society of Australia | Cambridge Core](https://static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary-alt:20170407143734-00812-mediumThumb-S1323358016000114_fig10g.jpg?pub-status=live)
The Disc Origin of the Milky Way Bulge | Publications of the Astronomical Society of Australia | Cambridge Core
![PDF) The SPHINX M-dwarf Spectral Grid. I. Benchmarking New Model Atmospheres to Derive Fundamental M-dwarf Properties PDF) The SPHINX M-dwarf Spectral Grid. I. Benchmarking New Model Atmospheres to Derive Fundamental M-dwarf Properties](https://i1.rgstatic.net/publication/368427799_The_SPHINX_M-dwarf_Spectral_Grid_I_Benchmarking_New_Model_Atmospheres_to_Derive_Fundamental_M-dwarf_Properties/links/63e84e98e2e1515b6b8be032/largepreview.png)
PDF) The SPHINX M-dwarf Spectral Grid. I. Benchmarking New Model Atmospheres to Derive Fundamental M-dwarf Properties
This is an Open Access document downloaded from ORCA, Cardiff University's institutional repository: https://orca.cardiff.ac.uk/
GEOWISSENSCHAFTLICHE MITTEILUNGEN Proceedings of the 18th European VLBI for Geodesy and Astrometry Working Meeting 12-13 April
![Blue Book, The By Compilation - Book Sheet Music For Rudimental Solos - Buy Print Music TA.TSPB-20 | Sheet Music Plus Blue Book, The By Compilation - Book Sheet Music For Rudimental Solos - Buy Print Music TA.TSPB-20 | Sheet Music Plus](https://d29ci68ykuu27r.cloudfront.net/items/19746311/look_insides/large_file/file_2_page_1.png)
Blue Book, The By Compilation - Book Sheet Music For Rudimental Solos - Buy Print Music TA.TSPB-20 | Sheet Music Plus
![PDF) Galaxy and Mass Assembly (GAMA): Witnessing the assembly of the cluster Abell 1882 | Aaron Robotham - Academia.edu PDF) Galaxy and Mass Assembly (GAMA): Witnessing the assembly of the cluster Abell 1882 | Aaron Robotham - Academia.edu](https://0.academia-photos.com/attachment_thumbnails/31704832/mini_magick20190426-11542-1mh6slu.png?1556263331)
PDF) Galaxy and Mass Assembly (GAMA): Witnessing the assembly of the cluster Abell 1882 | Aaron Robotham - Academia.edu
![PDF) Critical tests of stellar evolution in open clusters | Birgitta Nordström and S. Meibom - Academia.edu PDF) Critical tests of stellar evolution in open clusters | Birgitta Nordström and S. Meibom - Academia.edu](https://0.academia-photos.com/attachment_thumbnails/39595542/mini_magick20190222-27921-12kfepy.png?1550879347)
PDF) Critical tests of stellar evolution in open clusters | Birgitta Nordström and S. Meibom - Academia.edu
![PDF) The MBHBM ⋆ Project. I. Measurement of the Central Black Hole Mass in Spiral Galaxy NGC 3504 Using Molecular Gas Kinematics PDF) The MBHBM ⋆ Project. I. Measurement of the Central Black Hole Mass in Spiral Galaxy NGC 3504 Using Molecular Gas Kinematics](https://i1.rgstatic.net/publication/340287229_The_MBHBM_Project_I_Measurement_of_the_Central_Black_Hole_Mass_in_Spiral_Galaxy_NGC_3504_Using_Molecular_Gas_Kinematics/links/5e8bbf80a6fdcca789fbddf2/largepreview.png)