व्हाइट द्वार्फ Meaning in English
व्हाइट द्वार्फ शब्द का अंग्रेजी अर्थ : white dwarf
ऐसे ही कुछ और शब्द
सफेद धारसफेद एल्डर
सफेद हाथी
सफेद एल्म
सफेद सदाबहार
सफेद झूठी इंडिगो
सफेद फेल्डस्पार
सफ़ेद एफआईआर
सफेद प्राथमिकी
श्वेत ध्वज
सफेद झंडा
सफ़ेद फूलों वाला
केक वगैरह पर की सफेद तह
सफेद बल
सफेद ग्लोब लिली
व्हाइट-द्वार्फ हिंदी उपयोग और उदाहरण
"" इस बीच ये व्हाइट द्वार्फ़ पर अपने स्वतंत्र व दौलत सिंह कोठारी के संग संयुक्त कार्य में संलग्न रहे।
व्हाइट-द्वार्फ इसके अंग्रेजी अर्थ का उदाहरण
Past research projects included research on white dwarf stars and examining the large-scale structure of galaxies.
Jay family In astroparticle physics, an Urca process is a reaction which emits a neutrino and which is assumed to take part in cooling processes in neutron stars and white dwarfs.
32 times that of the Sun, this star will end its life as a white dwarf.
Historically, it has been held that these X-rays might be excited by matter originating from the star, from a hot wind or a disk around the star, accreting onto the surface of a degenerate companion, such as a white dwarf or neutron star.
For example, it is not clear that enough matter can be accreted by a white dwarf, at the distance of the purported secondary star implied by the orbital period, sufficient to power an X-ray emission of nearly 1033 erg/s or 100 YW.
The binary nature of this system was announced in 1980 by Erika Böhm-Vitense based on an ultraviolet excess attributed to a white dwarf companion.
Pan-STARRS will also measure proper motion and parallax and should thereby discover many brown dwarfs, white dwarfs, and other nearby faint objects, and it should be able to conduct a complete census of all stars within 100 parsecs of the Sun.
Among the dimmest stars in the cluster are groups of white dwarfs that are 6 billion years old and another group that appear to be 4 billion years old.
Though planetary formation is perhaps unlikely as long as the disk is in active accretion, it may proceed apace once Mira A completes its red giant phase and becomes a white dwarf remnant.
7 solar masses, rather than a white dwarf as first envisioned.
However, a 2010 analysis of rapid optical brightness variations has indicated that Mira B is in fact a white dwarf.
* Compact objects – this subdiscipline studies very dense matter in white dwarfs and neutron stars and their effects on environments including accretion.
** Pulsating white dwarf.
* Timeline of white dwarfs, neutron stars, and supernovae.