dc.contributor.author |
Parthasarathy, M |
|
dc.date.accessioned |
2013-09-04T16:45:38Z |
|
dc.date.available |
2013-09-04T16:45:38Z |
|
dc.date.issued |
2024-01 |
|
dc.identifier.citation |
Research Notes of the AAS, Vol. 8, No. 1, 23 |
en |
dc.identifier.issn |
2515-5172 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/6325 |
|
dc.description |
Open Access |
en |
dc.description |
Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. |
|
dc.description.abstract |
As part of an ongoing search for hypervelocity stars I found seventeen two micron all sky survey sources with Gaia G magnitudes less than 16.0 and radial velocities less than -600 km s-1. All these stars are brighter in the K band when compared with their V and G magnitudes. Ten of these (including three carbon stars) are long period variable stars of Mira type. One is a relatively nearby high proper motion star and one is a very high galactic latitude chemically peculiar metal-poor star. It may be a galactic halo star. One star is a Kepler red giant, two stars may be cluster members and two are in the star-forming region (probably YSOs). It is not clear how these stars acquired such high radial velocities. Further study of these seventeen stars is needed. |
en |
dc.language.iso |
en |
en |
dc.publisher |
American Astronomical Society |
en |
dc.relation.uri |
https://iopscience.iop.org/article/10.3847/2515-5172/ad1ee7 |
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dc.rights |
© 2024. The Author(s). |
en |
dc.subject |
Hypervelocity stars |
en |
dc.title |
Seventeen 2 Micron All Sky Survey (2MASS) Hypervelocity Stars (HVS) from Gaia DR3 |
en |
dc.type |
Article |
en |