| | |
| | |
Stat |
Members: 3645 Articles: 2'504'928 Articles rated: 2609
26 April 2024 |
|
| | | |
|
Article overview
| |
|
Detection of White Dwarf Companions to Blue Straggler Stars from UVIT Observations of M67 | Sindhu N
; Annapurni Subramaniam
; Aaron M Geller
; Vikrant Jadhav
; Christian Knigge
; Mirko Simunovic
; Nathan Leigh
; Michael Shara
; Thomas H Puzia
; | Date: |
5 Aug 2019 | Abstract: | We investigate the old open cluster M67 using ultraviolet photometric data of
Ultra-Violet Imaging Telescope in multi-filter far-UV bands. M67, well known
for the presence of several blue straggler stars (BSS), has been put to
detailed tests to understand their formation pathways. Currently, there are
three accepted formation channels: mass transfer due to Roche-lobe overflow in
binary systems, stellar mergers either due to dynamical collisions or through
coalescence of close binaries. So far, there had not been any confirmed
detection of a white dwarf (WD) companion to any of the BSSs in this cluster.
Here, we present the detection of WD companions to 5 bright BSSs in M67. The
multiwavelength spectral energy distributions covering 0.12 -11.5 $mu$m range,
were found to require binary spectral fits for 5 BSSs, consisting of a cool
(BSS) and a hot companion. The parameters (Luminosity, Temperature, Radius and
Mass) of the hot companions suggest them to be WDs with mass in the range 0.2 -
0.35 M$_{odot}$ with T$_{eff}$ $sim$ 11000 - 24000 K. | Source: | arXiv, 1908.1573 | Services: | Forum | Review | PDF | Favorites |
|
|
No review found.
Did you like this article?
Note: answers to reviews or questions about the article must be posted in the forum section.
Authors are not allowed to review their own article. They can use the forum section.
browser Mozilla/5.0 AppleWebKit/537.36 (KHTML, like Gecko; compatible; ClaudeBot/1.0; +claudebot@anthropic.com)
|
| |
|
|
|
| News, job offers and information for researchers and scientists:
| |