User talk:U-95

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Disambiguation link notification for December 26
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 * Habitability of red dwarf systems (check to confirm | fix with Dab solver)
 * added a link pointing to Blue dwarf


 * NGC 4550 (check to confirm | fix with Dab solver)
 * added a link pointing to Mega


 * NGC 4654 (check to confirm | fix with Dab solver)
 * added a link pointing to Mega


 * Red dwarf (check to confirm | fix with Dab solver)
 * added a link pointing to Blue dwarf


 * Westerhout 31 (check to confirm | fix with Dab solver)
 * added a link pointing to Kilo


 * Westerhout 43 (check to confirm | fix with Dab solver)
 * added a link pointing to Kilo

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A page you started has been reviewed!
Thanks for creating V1427 Aquilae, U-95!

Wikipedia editor Ana Bykova just reviewed your page, and wrote this note for you:

Thank you for making a wiki page, it looks great. Please refer to the tags added to find out how you could improve it. Best wishes, Anastasia Bykova (talk) 00:46, 29 December 2012 (UTC)

To reply, leave a comment on Ana Bykova's talk page.

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Message
I have added your name here. There is some confusion on the image (more clearly, is it really image of the star?), I asked there to check the image, see if you can help there! --Tito Dutta (talk) 20:08, 31 December 2012 (UTC)
 * Did you mean this article? --Tito Dutta (talk) 20:11, 31 December 2012 (UTC)

DYK for HD 179821
The DYK project (nominate) 12:03, 3 January 2013 (UTC)

Disambiguation link notification for July 22
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Physical characteristics part for UY Scuti
Hi, U-95! I appreciate your effort in improving my article. First of all, thanks for adding me a reliable source. But moving the "Physical characteristics" part of my article UY Scuti makes the main meaning more shorter and uglier. Also, the size of the star does not have any physical significance to the characteristics of the star. When we talk about characteristic of the star, we only include its initial properties (i.e: mass, luminosity, temperature). Thank you! You can talk to me if you have any questions! --Johndric Valdez (talk) 12:53, 19 September 2013 (UTC)--

Anyway, why did you remove the "Physical characteristics" part? The size of the star gives the reader the impression of the star, then giving the physical characteristics or other details about it. I guess you just need to think about it. Before you make a change, talk to me. --Johndric Valdez (talk) 06:19, 20 September 2013 (UTC)--

PZ Cassiopeiae
You've updated the size of this star from the recently published paper, but I am unable to find any reference to the number 1400 that you quote. Quite likely it isn't given explicitly in the paper, but I am also unable to derive it from the given luminosities and effective temperature. I get a value of 1287 from the quoted 3600K and luminosity 250,000 times solar. Or 1261-1337 using the full range of luminosity estimates. Lithopsian (talk) 00:13, 27 December 2013 (UTC)

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Reference errors on 29 April
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Nomination of Tau Ceti e for deletion
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Nomination of Tau Ceti f for deletion
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Proposed deletion of Frozen star (hypothetical star)


The article Frozen star (hypothetical star) has been proposed for deletion&#32;because of the following concern: "Not even in the same galaxy as notable concepts in astrophysics. 'Frozen star' appears literally in a single sentence of Ref. 2, and not at all in Ref. 1. A search on google Scholar gets me results only about black holes, not frozen stars in this sense."

While all constructive contributions to Wikipedia are appreciated, pages may be deleted for any of several reasons.

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Please consider improving the page to address the issues raised. Removing will stop the proposed deletion process, but other deletion processes exist. In particular, the speedy deletion process can result in deletion without discussion, and articles for deletion allows discussion to reach consensus for deletion. Tercer (talk) 19:05, 11 July 2021 (UTC)