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| MSC 319.9-0.7 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST20:15:00 |
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trying to find the most relevant references on this object.
More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
1996A&AS..118..329W 
|
96 | 279 | The MOST supernova remnant catalogue (MSC). | WHITEOAK J.B.Z. and GREEN A.J. | |||||
| 2007A&A...470..965H | 473 | A | X C | 12 | 4 | 13 | Radio and X-ray nebulae associated with PSR J1509-5850. | HUI C.Y. and BECKER W. | |
| 2010ApJ...712..596N | 1678 | S X C F | 41 | 11 | 21 | Radio polarization observations of G319.9-0.7: a bow-shock nebula with an azimuthal magnetic field powered by pulsar J1509-5850. | NG C.-Y., GAENSLER B.M., CHATTERJEE S., et al. | ||
| 2012ApJ...746..105N | 132 | D | X | 4 | 22 | 16 | An extreme pulsar tail protruding from the Frying Pan supernova remnant. | NG C.-Y., BUCCIANTINI N., GAENSLER B.M., et al. | |
| 2016ApJ...820..100M | 80 | X | 2 | 19 | 12 | Radio polarization observations of the snail: a crushed pulsar wind nebula in G327.1-1.1 with a highly ordered magnetic field. | MA Y.K., NG C.-Y., BUCCIANTINI N., et al. | ||
| 2017ApJ...842..100N | 81 | X | 2 | 17 | 1 | Discovery of a synchrotron bubble associated with PSR J1015-5719. | NG C.-Y., BANDIERA R., HUNSTEAD R.W., et al. | ||
| 2018MNRAS.477L..66M | 41 | X | 1 | 9 | ~ | Discovery of a radio nebula around PSR J0855-4644. | MAITRA C., ROY S., ACERO F., et al. | ||
| 2021MNRAS.504.4952A | 17 | D | 1 | 51 | ~ | Maximally hard radio spectra from Fermi acceleration in pulsar-wind nebulae. | ARAD O., LAVI A. and KESHET U. | ||
| 2022MNRAS.509.4143Z | 18 | D | 1 | 79 | ~ | Radio and X-ray spectral properties of gamma-ray bursts and pulsar wind nebulae. | ZHU B.-T., LU F.-W., ZHOU B., et al. | ||
| 2023ApJ...945...82L | 93 | X | 2 | 16 | ~ | Radio Study of the Pulsar Wind Nebula Powered by PSR B1706-44. | LIU Y.H., NG C.-Y. and DODSON R. |
