| | |
| | |
Stat |
Members: 3645 Articles: 2'503'724 Articles rated: 2609
24 April 2024 |
|
| | | |
|
Article overview
| |
|
Mass Limit on Nemesis | Varun Bhalerao
; M. N. Vahia
; | Date: |
20 Feb 2005 | Subject: | astro-ph | Affiliation: | Indian Institute of Technology Bombay, TIFR | Abstract: | We assume that if the sun has a companion, it has a period of 27 Myr corresponding to the periodicity seen in cometary impacts on earth. Based on this assumption, it is seen that the inner Lagrengian point of the interaction between the Sun and its companion is in the Oort cloud. From this we calculate the mass -- distance relation for the companion. We then compute the expected apparent magnitude (visible and J band) for the companion using the models of Burrows (1993). We then compare this with the catalogue completeness of optical and infrared catalogues to show that the sun cannot have a companion of mass greater than 44 M_jup (0.042 M_sun) | Source: | arXiv, astro-ph/0502390 | 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:
| |